[
    {
        "id": "authors:avera-s5s35",
        "collection": "authors",
        "collection_id": "avera-s5s35",
        "cite_using_url": "https://authors.library.caltech.edu/records/avera-s5s35",
        "type": "article",
        "title": "Online learning of eddy-viscosity and backscattering closures for geophysical turbulence using ensemble Kalman inversion",
        "author": [
            {
                "family_name": "Guan",
                "given_name": "Yifei",
                "orcid": "0000-0003-2070-3654"
            },
            {
                "family_name": "Hassanzadeh",
                "given_name": "Pedram",
                "orcid": "0000-0001-9425-8085"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Huang",
                "given_name": "Daniel Zhengyu"
            },
            {
                "family_name": "Wu",
                "given_name": "Jinlong",
                "orcid": "0000-0001-7438-4228"
            },
            {
                "family_name": "Lopez-Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895"
            }
        ],
        "abstract": "<p>Different approaches to using data-driven methods for subgrid-scale closure modeling of geophysical turbulence have emerged recently. Most of these approaches are data hungry and lack interpretability and out-of-distribution generalizability. Here, we use a hybrid approach that combines turbulence theory, physics-based modeling, and data-driven methods to overcome these challenges. Specifically, we address the parametric uncertainty of well-known physics-based large-eddy simulation (LES) closures: the Smagorinsky (Smag) and Leith eddy-viscosity models (one free parameter) and the Jansen-Held (JH) backscattering model (two free parameters). For various cases of two-dimensional turbulence, optimal parameters are first learned online from data via ensemble Kalman inversion (EKI), such that for each case, the LES energy spectrum matches that of direct numerical simulation (DNS). We quantify the uncertainties on these parameters using a modern machine-learning-accelerated Bayesian workflow, \", , \" Only a small training dataset is needed (to calculate the DNS spectra); i.e., the approach is data-efficient. We find the optimized parameter(s) and their associated uncertainty for each closure to be constant across broad flow regimes that differ in dominant length scales, eddy/jet structures, and dynamics, suggesting that these closures are generalizable. Next, we show that the online learned constants agree with the predictions of a recent semianalytical derivation, providing further interpretability. In both and tests that include examining the extreme events, LES with optimized closures, especially with JH, outperforms the baselines (LES with standard Smag, dynamic Smag, or Leith). This work shows the promise of combining advances in theory, physics-based modeling (e.g., JH), and data-driven modeling (e.g., online learning with EKI) to develop data-efficient frameworks for accurate, interpretable, and generalizable closures for geophysical turbulence, with ultimate applications in weather and climate prediction.</p>",
        "doi": "10.1103/mnbm-3g56",
        "issn": "2643-1564",
        "publisher": "American Physical Society",
        "publication": "Physical Review Research",
        "publication_date": "2026-05-27",
        "series_number": "2",
        "volume": "8",
        "issue": "2",
        "pages": "023215"
    },
    {
        "id": "authors:4jy0k-xx805",
        "collection": "authors",
        "collection_id": "4jy0k-xx805",
        "cite_using_url": "https://authors.library.caltech.edu/records/4jy0k-xx805",
        "type": "article",
        "title": "Thank You to Our 2025 Peer Reviewers",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391"
            },
            {
                "family_name": "MacBean",
                "given_name": "Natasha",
                "orcid": "0000-0001-6797-4836"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Grooms",
                "given_name": "Ian",
                "orcid": "0000-0002-4678-7203"
            }
        ],
        "abstract": "<p>The editors of Journal of Advances in Modeling Earth Systems thank the 1,035 reviewers who provided 1,649 reviews during 2025. Their hard work and insights, typically done anonymously, benefits authors, readers, and the broader science community.</p>",
        "doi": "10.1029/2026ms006024",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth System (JAMES)",
        "publication_date": "2026-05",
        "series_number": "5",
        "volume": "18",
        "issue": "5",
        "pages": "e2026MS006024"
    },
    {
        "id": "authors:ktk32-whm45",
        "collection": "authors",
        "collection_id": "ktk32-whm45",
        "cite_using_url": "https://authors.library.caltech.edu/records/ktk32-whm45",
        "type": "article",
        "title": "Reconciling Jupiter's vertical motions with the observed cloud structure in the upper troposphere",
        "author": [
            {
                "family_name": "Mendon\u00e7a",
                "given_name": "Jo\u00e3o M.",
                "orcid": "0000-0002-6907-4476"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Lian",
                "given_name": "Yuan",
                "orcid": "0000-0003-1776-291X"
            }
        ],
        "abstract": "<div class=\"Abstracts u-font-serif\">\n<div class=\"abstract author\">\n<div>\n<div class=\"u-margin-s-bottom\">The eddy fluxes of angular momentum in Jupiter&rsquo;s upper troposphere are known to converge in prograde jets and diverge in retrograde jets. Away from the equator, this implies convergence of the Eulerian mean meridional flow in zones (anticyclonic shear) and divergence in belts (cyclonic shear). It indicates lower-tropospheric downwelling in zones and upwelling in belts because the mean meridional circulation almost certainly closes at depth. Yet the observed banded structure of Jupiter&rsquo;s clouds and hazes suggests that there is upwelling in the brighter zones and downwelling in the darker belts. Here, we show that this apparent contradiction can be resolved by considering not the Eulerian but the transformed Eulerian mean circulation, which includes a Stokes drift owing to eddies and is a better approximation of the Lagrangian mean transport of tracers such as ammonia. The potential vorticity structure inferred from observations paired with mixing length arguments suggests that there is transformed Eulerian mean upwelling in zones and downwelling in belts. Simulations with a global circulation model of Jupiter&rsquo;s upper atmosphere demonstrate the plausibility of these inferences and allow us to speculate on the band structure at deeper levels.</div>\n</div>\n</div>\n</div>",
        "doi": "10.1016/j.icarus.2025.116766",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2026-01-01",
        "volume": "443",
        "pages": "116766"
    },
    {
        "id": "authors:dctqh-4aa10",
        "collection": "authors",
        "collection_id": "dctqh-4aa10",
        "cite_using_url": "https://authors.library.caltech.edu/records/dctqh-4aa10",
        "type": "article",
        "title": "ClimaLand: A Land Surface Model Designed to Enable Data-Driven Parameterizations",
        "author": [
            {
                "family_name": "Deck",
                "given_name": "Katherine",
                "orcid": "0009-0001-0572-7642",
                "clpid": "Deck-Katherine"
            },
            {
                "family_name": "Braghiere",
                "given_name": "Renato K.",
                "orcid": "0000-0002-7722-717X",
                "clpid": "Braghiere-Renato-K"
            },
            {
                "family_name": "Renchon",
                "given_name": "Alexandre A.",
                "orcid": "0000-0002-9521-5092",
                "clpid": "Renchon-Alexandre-A"
            },
            {
                "family_name": "Sloan",
                "given_name": "Julia",
                "orcid": "0000-0003-0200-063X",
                "clpid": "Sloan-Julia"
            },
            {
                "family_name": "Bozzola",
                "given_name": "Gabriele",
                "orcid": "0000-0003-3696-6408",
                "clpid": "Bozzola-Gabriele"
            },
            {
                "family_name": "Speer",
                "given_name": "Edward",
                "clpid": "Speer-Edward"
            },
            {
                "family_name": "Ben Mackay",
                "given_name": "J."
            },
            {
                "family_name": "Reddy",
                "given_name": "Teja",
                "orcid": "0009-0004-3319-825X",
                "clpid": "Reddy-Teja"
            },
            {
                "family_name": "Phan",
                "given_name": "Kevin",
                "clpid": "Phan-Kevin"
            },
            {
                "family_name": "Gagn\u00e9\u2010Landmann",
                "given_name": "Anna L."
            },
            {
                "family_name": "Li",
                "given_name": "Yuchen",
                "orcid": "0000-0002-7518-5359"
            },
            {
                "family_name": "Yatunin",
                "given_name": "Dennis",
                "clpid": "Yatunin-Dennis"
            },
            {
                "family_name": "Charbonneau",
                "given_name": "Andrew",
                "clpid": "Charbonneau-Andrew"
            },
            {
                "family_name": "Efrat\u2010Henrici",
                "given_name": "Nat",
                "clpid": "Efrat\u2010Henrici-Nat"
            },
            {
                "family_name": "Bach",
                "given_name": "Eviatar",
                "orcid": "0000-0002-9725-0203",
                "clpid": "Bach-Eviatar"
            },
            {
                "family_name": "Ma",
                "given_name": "Shuang",
                "orcid": "0000-0002-6494-724X",
                "clpid": "Ma-Shuang"
            },
            {
                "family_name": "Gentine",
                "given_name": "Pierre",
                "orcid": "0000-0002-0845-8345"
            },
            {
                "family_name": "Frankenberg",
                "given_name": "Christian",
                "orcid": "0000-0002-0546-5857",
                "clpid": "Frankenberg-C"
            },
            {
                "family_name": "Bloom",
                "given_name": "A. Anthony",
                "orcid": "0000-0002-1486-1499",
                "clpid": "Bloom-A-Anthony"
            },
            {
                "family_name": "Wang",
                "given_name": "Yujie",
                "orcid": "0000-0002-3729-2743",
                "clpid": "Wang-Yujie"
            },
            {
                "family_name": "Longo",
                "given_name": "Marcos",
                "orcid": "0000-0001-5062-6245"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>Land surface models (LSMs) are essential tools for simulating the coupled climate system, representing the dynamics of water, energy, and carbon fluxes on land and their interaction with the atmosphere. However, parameterizing sub\u2010grid processes at the scales relevant to climate models (~10&ndash;100 km) remains a considerable challenge. The parameterizations typically have a large number of unknown and often correlated parameters, making calibration and uncertainty quantification difficult. Moreover, many existing LSMs are not readily adaptable to the incorporation of modern machine learning (ML) parameterizations trained with in situ and satellite data. This article presents the first version of ClimaLand, a new LSM designed for overcoming these limitations, including a description of the core equations underlying the model, the results of an extensive set of validation exercises, and an assessment of the computational performance of the model. We show that ClimaLand can leverage graphics processing units for computational efficiency, and that its modular architecture and high\u2010level programming language, Julia, allows for integration with ML libraries. In the future, this will enable efficient simulation, calibration, and uncertainty quantification with ClimaLand.</p>",
        "doi": "10.1029/2025ms005118",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth System (JAMES)",
        "publication_date": "2026-01",
        "series_number": "1",
        "volume": "18",
        "issue": "1",
        "pages": "e2025MS005118"
    },
    {
        "id": "authors:ksr6w-qkg20",
        "collection": "authors",
        "collection_id": "ksr6w-qkg20",
        "cite_using_url": "https://authors.library.caltech.edu/records/ksr6w-qkg20",
        "type": "article",
        "title": "An Energetic Framework for Understanding Hadley Circulation Width Variations: Seasonal Cycle, ENSO, and Global Warming",
        "author": [
            {
                "family_name": "Khapikova",
                "given_name": "Polina",
                "clpid": "Khapikova-Polina"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>The Hadley Circulation (HC), a dominant driver of energy and moisture transport in low latitudes, varies in meridional extent on timescales ranging from seasonal to multidecadal. For example, the subtropical termini of the descending HC branches shift latitudinally by 10&deg; over the seasonal cycle, contrasting with a 34&deg; seasonal shift of the Intertropical Convergence Zone (ITCZ). While diagnostic energetic frameworks have successfully provided insight into ITCZ migrations, this study applies a similar framework to understand HC extent variations across timescales. The framework relates the HC extent to the tropical net energy input (NEI) and the eddy energy export from the HC to the extratropics. Variations in HC extent can therefore be decomposed into contributions from NEI and eddy energy export changes, which play different roles on different timescales. Analysis of observations and climate simulations shows that HC contraction during El Ni&ntilde;o is primarily related to increased tropical NEI, while HC expansion under global warming is primarily related to increased eddy energy export. This energetic framework, while not fully predictive because it excludes factors such as the angular momentum balance, offers a new perspective for understanding variations in HC extent.</p>",
        "doi": "10.1175/jas-d-25-0052.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2025-11-01",
        "series_number": "11",
        "volume": "82",
        "issue": "11",
        "pages": "2569-2580"
    },
    {
        "id": "authors:2p7vy-b4x13",
        "collection": "authors",
        "collection_id": "2p7vy-b4x13",
        "cite_using_url": "https://authors.library.caltech.edu/records/2p7vy-b4x13",
        "type": "article",
        "title": "A Physics-Constrained Neural Differential Equation Framework for Data-Driven Snowpack Simulation",
        "author": [
            {
                "family_name": "Charbonneau",
                "given_name": "Andrew",
                "clpid": "Charbonneau-Andrew"
            },
            {
                "family_name": "Deck",
                "given_name": "Katherine",
                "clpid": "Deck-Katherine"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>This paper presents a physics-constrained neural differential equation framework for parameterization and employs it to model the time evolution of seasonal snow depth given hydrometeorological forcings. When trained on data from multiple SNOTEL sites, the parameterization predicts daily snow depth with under 9% median error and Nash&ndash;Sutcliffe efficiencies over 0.94 across a wide variety of snow climates. The parameterization also generalizes to new sites not seen during training, which is not often true for calibrated snow models. Requiring the parameterization to predict snow water equivalent in addition to snow depth only increases the error to &sim;12%. The structure of the approach guarantees the satisfaction of physical constraints, enables these constraints during model training, and allows modeling at different temporal resolutions without additional retraining of the parameterization. These benefits hold potential in climate modeling and could extend to other dynamical systems with physical constraints.</p>",
        "doi": "10.1175/aies-d-24-0040.1",
        "issn": "2769-7525",
        "publisher": "American Meteorological Society",
        "publication": "Artificial Intelligence for the Earth Systems",
        "publication_date": "2025-07",
        "series_number": "3",
        "volume": "4",
        "issue": "3",
        "pages": "e240040"
    },
    {
        "id": "authors:fa0bx-54d29",
        "collection": "authors",
        "collection_id": "fa0bx-54d29",
        "cite_using_url": "https://authors.library.caltech.edu/records/fa0bx-54d29",
        "type": "article",
        "title": "Observational constraints imply limited future Atlantic meridional overturning circulation weakening",
        "author": [
            {
                "family_name": "Bonan",
                "given_name": "David B.",
                "orcid": "0000-0003-3867-6009",
                "clpid": "Bonan-David-B"
            },
            {
                "family_name": "Thompson",
                "given_name": "Andrew F.",
                "orcid": "0000-0003-0322-4811",
                "clpid": "Thompson-A-F"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Zanna",
                "given_name": "Laure",
                "orcid": "0000-0002-8472-4828"
            },
            {
                "family_name": "Armour",
                "given_name": "Kyle C.",
                "orcid": "0000-0002-6833-5179"
            },
            {
                "family_name": "Sun",
                "given_name": "Shantong"
            }
        ],
        "abstract": "<p>The degree to which the Atlantic meridional overturning circulation (AMOC) weakens over the twenty-first century varies widely across climate models, with some predicting substantial weakening. Here we show that this uncertainty can be greatly reduced by using a thermal-wind expression that relates the AMOC strength to the meridional density difference and the overturning depth in the Atlantic. This expression captures the intermodel spread in AMOC weakening, with most of the spread arising from overturning depth changes. The overturning depth also establishes a crucial link between the present-day and future AMOC strength. Climate models with a stronger and deeper present-day overturning tend to predict larger weakening and shoaling under warming because the present-day North Atlantic is less stratified, allowing for a deeper penetration of surface buoyancy flux changes, larger density changes at depth and, consequently, larger AMOC weakening. By incorporating observational constraints, we conclude that the AMOC will experience limited weakening of about 3&ndash;6&thinsp;Sv (about 18&ndash;43%) by the end of this century, regardless of emissions scenario. These results indicate that the uncertainty in twenty-first-century AMOC weakening and the propensity to predict substantial AMOC weakening can be attributed primarily to climate model biases in accurately simulating the present-day ocean stratification.</p>",
        "doi": "10.1038/s41561-025-01709-0",
        "issn": "1752-0894",
        "publisher": "Nature Publishing Group",
        "publication": "Nature Geoscience",
        "publication_date": "2025-06",
        "series_number": "6",
        "volume": "18",
        "issue": "6",
        "pages": "479-487"
    },
    {
        "id": "authors:wz2n2-t4m23",
        "collection": "authors",
        "collection_id": "wz2n2-t4m23",
        "cite_using_url": "https://authors.library.caltech.edu/records/wz2n2-t4m23",
        "type": "article",
        "title": "Impacts of leaf traits on vegetation optical properties in Earth system modeling",
        "author": [
            {
                "family_name": "Wang",
                "given_name": "Yujie",
                "orcid": "0000-0002-3729-2743",
                "clpid": "Wang-Yujie"
            },
            {
                "family_name": "Braghiere",
                "given_name": "Renato K.",
                "orcid": "0000-0002-7722-717X",
                "clpid": "Braghiere-Renato-K"
            },
            {
                "family_name": "Fischer",
                "given_name": "Woodward W.",
                "orcid": "0000-0002-8836-3054",
                "clpid": "Fischer-W-W"
            },
            {
                "family_name": "Yao",
                "given_name": "Yitong",
                "orcid": "0000-0002-1713-6719",
                "clpid": "Yao-Yitong"
            },
            {
                "family_name": "Shen",
                "given_name": "Zhaoyi",
                "orcid": "0000-0002-0444-4720",
                "clpid": "Shen-Zhaoyi"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bloom",
                "given_name": "A. Anthony",
                "orcid": "0000-0002-1486-1499",
                "clpid": "Bloom-A-Anthony"
            },
            {
                "family_name": "Schimel",
                "given_name": "David",
                "orcid": "0000-0003-3473-8065",
                "clpid": "Schimel-David"
            },
            {
                "family_name": "Croft",
                "given_name": "Holly"
            },
            {
                "family_name": "Winkler",
                "given_name": "Alexander J.",
                "orcid": "0000-0001-6574-4471"
            },
            {
                "family_name": "Reichstein",
                "given_name": "Markus",
                "orcid": "0000-0001-5736-1112"
            },
            {
                "family_name": "Frankenberg",
                "given_name": "Christian",
                "orcid": "0000-0002-0546-5857",
                "clpid": "Frankenberg-C"
            }
        ],
        "abstract": "<div class=\"c-article-section\">\n<div class=\"c-article-section__content\">\n<p>Quantifying surface energy and carbon budgets is essential for projecting Earth&rsquo;s climate. Earth System Models (ESMs) typically simulate land surface processes based on plant functional types (PFTs), neglecting the diversity of plant functional traits or characteristics (PFCs; e.g., chlorophyll content and leaf mass per area). Here, we demonstrate substantial differences in modeled leaf optical properties (LOP) and surface albedo between traditional PFT-based and PFC-based approaches, particularly in tropical and boreal forests. We configure the canopy radiative transfer scheme in the Community Earth System Model using PFC-based LOP. This new configuration produces lower shortwave surface albedo in the tropics but higher albedo in boreal regions (&gt;5&thinsp;W&thinsp;m<sup>&minus;2</sup> radiative flux differences), and a weaker tropical but stronger boreal carbon sink. Through land-atmosphere coupling, the PFC-based configuration further alters atmospheric processes, leading to different temperature, cloud cover, and precipitation patterns. Our findings highlight the need to move beyond traditional PFT-based approaches in ESMs.</p>\n</div>\n</div>",
        "doi": "10.1038/s41467-025-60149-x",
        "pmcid": "PMC12119829",
        "issn": "2041-1723",
        "publisher": "Nature Publishing Group",
        "publication": "Nature Communications",
        "publication_date": "2025-05-29",
        "series_number": "1",
        "volume": "16",
        "issue": "1",
        "pages": "4968"
    },
    {
        "id": "authors:8kb8h-vv697",
        "collection": "authors",
        "collection_id": "8kb8h-vv697",
        "cite_using_url": "https://authors.library.caltech.edu/records/8kb8h-vv697",
        "type": "article",
        "title": "Dynamical-generative downscaling of climate model ensembles",
        "author": [
            {
                "family_name": "Lopez-Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895"
            },
            {
                "family_name": "Wan",
                "given_name": "Zhong Yi"
            },
            {
                "family_name": "Zepeda-N\u00fa\u00f1ez",
                "given_name": "Leonardo"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Anderson",
                "given_name": "John"
            },
            {
                "family_name": "Sha",
                "given_name": "Fei",
                "orcid": "0009-0006-1733-5482"
            }
        ],
        "abstract": "Regional high-resolution climate projections are crucial for many applications, such as agriculture, hydrology, and natural hazard risk assessment. Dynamical downscaling, the state-of-the-art method to produce localized future climate information, involves running a regional climate model (RCM) driven by an Earth System Model (ESM), but it is too computationally expensive to apply to large climate projection ensembles. We propose an approach combining dynamical downscaling with generative AI to reduce the cost and improve the uncertainty estimates of downscaled climate projections. In our framework, an RCM dynamically downscales ESM output to an intermediate resolution, followed by a generative diffusion model that further refines the resolution to the target scale. This approach leverages the generalizability of physics-based models and the sampling efficiency of diffusion models, enabling the downscaling of large multimodel ensembles. We evaluate our method against dynamically downscaled climate projections from the Coupled Model Intercomparison Project 6 (CMIP6) ensemble. Our results demonstrate its ability to provide more accurate uncertainty bounds on future regional climate than alternatives such as dynamical downscaling of smaller ensembles, or traditional empirical statistical downscaling methods. We also show that dynamical-generative downscaling results in significantly lower errors than popular statistical downscaling techniques, and captures more accurately the spectra, tail dependence, and multivariate correlations of meteorological fields. These characteristics make the dynamical-generative framework a flexible, accurate, and efficient way to downscale large ensembles of climate projections, currently out of reach for pure dynamical downscaling.",
        "doi": "10.1073/pnas.2420288122",
        "issn": "0027-8424",
        "publisher": "National Academy of Sciences",
        "publication": "Proceedings of the National Academy of Sciences",
        "publication_date": "2025-04-29",
        "series_number": "17",
        "volume": "122",
        "issue": "17",
        "pages": "e2420288122"
    },
    {
        "id": "authors:nxwxs-nn967",
        "collection": "authors",
        "collection_id": "nxwxs-nn967",
        "cite_using_url": "https://authors.library.caltech.edu/records/nxwxs-nn967",
        "type": "article",
        "title": "Changes in the Frequency of Observed Temperature Extremes Largely Driven by a Distribution Shift",
        "author": [
            {
                "family_name": "Patel",
                "given_name": "Ronak N.",
                "orcid": "0000-0002-5263-3411",
                "clpid": "Patel-Ronak-N"
            },
            {
                "family_name": "Bonan",
                "given_name": "David B.",
                "orcid": "0000-0003-3867-6009",
                "clpid": "Bonan-David-B"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>Extreme heat poses significant threats to human life and ecosystems. Quantifying the effects of anthropogenic climate change on extreme heat has remained challenging, in part due to the short observational record. Here, we isolate the most slowly varying component of the frequency at which the historical 90th and 99th percentiles were exceeded in observational records from 1955 to 2021 by using a statistical method called low\u2010frequency component analysis. The emerging spatiotemporal signal in the changing frequency of temperature extremes can be attributed to a shift of the temperature distribution by local warming of the annual\u2010mean daily maximum temperature. The shift explains over 80% of the interannual variability in the frequency at which the historical 90th percentile is exceeded in the tropics and up to 50% in higher latitudes. This work connects variability in the frequency of extreme surface temperatures to variability in mean local warming.</p>",
        "doi": "10.1029/2024gl110707",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2024-12-28",
        "series_number": "24",
        "volume": "51",
        "issue": "24",
        "pages": "e2024GL110707"
    },
    {
        "id": "authors:2x0kp-pkz30",
        "collection": "authors",
        "collection_id": "2x0kp-pkz30",
        "cite_using_url": "https://authors.library.caltech.edu/records/2x0kp-pkz30",
        "type": "article",
        "title": "Online Learning of Entrainment Closures in a Hybrid Machine Learning Parameterization",
        "author": [
            {
                "family_name": "Christopoulos",
                "given_name": "Costa",
                "orcid": "0000-0002-8552-465X",
                "clpid": "Christopoulos-Costa"
            },
            {
                "family_name": "Lopez\u2010Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895",
                "clpid": "Lopez\u2010Gomez-Ignacio"
            },
            {
                "family_name": "Beucler",
                "given_name": "Tom",
                "orcid": "0000-0002-5731-1040"
            },
            {
                "family_name": "Cohen",
                "given_name": "Yair",
                "orcid": "0000-0002-9615-2476",
                "clpid": "Cohen-Yair"
            },
            {
                "family_name": "Kawczynski",
                "given_name": "Charles",
                "clpid": "Kawczynski-Charles-N"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>This work integrates machine learning into an atmospheric parameterization to target uncertain mixing processes while maintaining interpretable, predictive, and well-established physical equations. We adopt an eddy-diffusivity mass-flux (EDMF) parameterization for the unified modeling of various convective and turbulent regimes. To avoid drift and instability that plague offline-trained machine learning parameterizations that are subsequently coupled with climate models, we frame learning as an inverse problem: Data-driven models are embedded within the EDMF parameterization and trained online in a one-dimensional vertical global climate model (GCM) column. Training is performed against output from large-eddy simulations (LES) forced with GCM-simulated large-scale conditions in the Pacific. Rather than optimizing subgrid-scale tendencies, our framework directly targets climate variables of interest, such as the vertical profiles of entropy and liquid water path. Specifically, we use ensemble Kalman inversion to simultaneously calibrate both the EDMF parameters and the parameters governing data-driven lateral mixing rates. The calibrated parameterization outperforms existing EDMF schemes, particularly in tropical and subtropical locations of the present climate, and maintains high fidelity in simulating shallow cumulus and stratocumulus regimes under increased sea surface temperatures from AMIP4K experiments. The results showcase the advantage of physically constraining data-driven models and directly targeting relevant variables through online learning to build robust and stable machine learning parameterizations.</p>",
        "doi": "10.1029/2024ms004485",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth System (JAMES)",
        "publication_date": "2024-11",
        "series_number": "11",
        "volume": "16",
        "issue": "11",
        "pages": "e2024MS004485"
    },
    {
        "id": "authors:ranze-1vf44",
        "collection": "authors",
        "collection_id": "ranze-1vf44",
        "cite_using_url": "https://authors.library.caltech.edu/records/ranze-1vf44",
        "type": "article",
        "title": "Learning about structural errors in models of complex dynamical systems",
        "author": [
            {
                "family_name": "Wu",
                "given_name": "Jin-Long",
                "orcid": "0000-0001-7438-4228",
                "clpid": "Wu-Jin-Long"
            },
            {
                "family_name": "Levine",
                "given_name": "Matthew E.",
                "clpid": "Levine-Matthew-E"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            }
        ],
        "abstract": "<div class=\"abstract author\">\n<div>\n<p>Complex dynamical systems are notoriously difficult to model because some degrees of freedom (e.g., small scales) may be computationally unresolvable or are incompletely understood, yet they are dynamically important. For example, the small scales of cloud dynamics and droplet formation are crucial for controlling climate, yet are unresolvable in global climate models. Semi-empirical closure models for the effects of unresolved degrees of freedom often exist and encode important domain-specific knowledge. Building on such closure models and correcting them through learning the structural errors can be an effective way of fusing data with domain knowledge. Here we describe a general approach, principles, and algorithms for learning about structural errors. Key to our approach is to include structural error models inside the models of complex systems, for example, in closure models for unresolved scales. The structural errors then map, usually nonlinearly, to observable data. As a result, however, mismatches between model output and data are only indirectly informative about structural errors, due to a lack of labeled pairs of inputs and outputs of structural error models. Additionally, derivatives of the model may not exist or be readily available. We discuss how structural error models can be learned from indirect data with derivative-free Kalman inversion algorithms and variants, how sparsity constraints enforce a &ldquo;do no harm&rdquo; principle, and various ways of modeling structural errors. We also discuss the merits of using non-local and/or stochastic error models. In addition, we demonstrate how data assimilation techniques can assist the learning about structural errors in non-ergodic systems. The concepts and algorithms are illustrated in two numerical examples based on the Lorenz-96 system and a human glucose-insulin model.</p>\n</div>\n</div>\n<div class=\"abstract graphical\"></div>",
        "doi": "10.1016/j.jcp.2024.113157",
        "issn": "0021-9991",
        "publisher": "Elsevier",
        "publication": "Journal of Computational Physics",
        "publication_date": "2024-09-15",
        "volume": "513",
        "pages": "113157"
    },
    {
        "id": "authors:z90g3-6pn61",
        "collection": "authors",
        "collection_id": "z90g3-6pn61",
        "cite_using_url": "https://authors.library.caltech.edu/records/z90g3-6pn61",
        "type": "article",
        "title": "Precipitation Over a Wide Range of Climates Simulated With Comprehensive GCMs",
        "author": [
            {
                "family_name": "Bonan",
                "given_name": "David B.",
                "orcid": "0000-0003-3867-6009",
                "clpid": "Bonan-David-B"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Zhu",
                "given_name": "Jiang",
                "orcid": "0000-0002-0908-5130"
            }
        ],
        "abstract": "<div class=\"article-section__content en main\">\n<p>Idealized general circulation models (GCMs) suggest global-mean precipitation ceases to increase with warming in hot climates because evaporation is limited by the available solar radiation at the surface. We investigate the extent to which this generalizes in comprehensive GCMs. We find that in the Community Atmosphere Model, global-mean precipitation increases approximately linearly with global-mean surface temperatures up to about 330&nbsp;K, where it peaks at 5&nbsp;mm&nbsp;day<sup>&minus;1</sup>. Beyond 330 K, global-mean precipitation decreases substantially despite increasing surface temperatures because of increased atmospheric shortwave absorption by water vapor, which decreases the shortwave radiation available for evaporation at the surface. Precipitation decreases in the tropics and subtropics but continues to increase in the extratropics because of continuously strengthening poleward moisture transport. Precipitable water increases everywhere, resulting in longer water-vapor residence times and implying more episodic precipitation. Other GCMs indicate global-mean precipitation might exhibit a smaller maximum rate and begin to decrease at lower surface temperatures.</p>\n</div>",
        "doi": "10.1029/2024gl109892",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2024-08-28",
        "series_number": "16",
        "volume": "51",
        "issue": "16",
        "pages": "e2024GL109892"
    },
    {
        "id": "authors:4b1se-d2h14",
        "collection": "authors",
        "collection_id": "4b1se-d2h14",
        "cite_using_url": "https://authors.library.caltech.edu/records/4b1se-d2h14",
        "type": "article",
        "title": "Training Warm-Rain Bulk Microphysics Schemes Using Super-Droplet Simulations",
        "author": [
            {
                "family_name": "Azimi",
                "given_name": "Sajjad",
                "orcid": "0000-0002-6329-7775",
                "clpid": "Azimi-Sajjad"
            },
            {
                "family_name": "Jaruga",
                "given_name": "Anna",
                "orcid": "0000-0003-3194-6440",
                "clpid": "Jaruga-Anna"
            },
            {
                "family_name": "de Jong",
                "given_name": "Emily",
                "orcid": "0000-0002-5310-4554",
                "clpid": "de-Jong-Emily"
            },
            {
                "family_name": "Arabas",
                "given_name": "Sylwester",
                "orcid": "0000-0003-2361-0082"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>Cloud microphysics is a critical aspect of the Earth's climate system, which involves processes at the nano\u2010 and micrometer scales of droplets and ice particles. In climate modeling, cloud microphysics is commonly represented by bulk models, which contain simplified process rates that require calibration. This study presents a framework for calibrating warm\u2010rain bulk schemes using high\u2010fidelity super\u2010droplet simulations that provide a more accurate and physically based representation of cloud and precipitation processes. The calibration framework employs ensemble Kalman methods including Ensemble Kalman Inversion and Unscented Kalman Inversion to calibrate bulk microphysics schemes with probabilistic super\u2010droplet simulations. We demonstrate the framework's effectiveness by calibrating a single\u2010moment bulk scheme, resulting in a reduction of data\u2010model mismatch by more than 75% compared to the model with initial parameters. Thus, this study demonstrates a powerful tool for enhancing the accuracy of bulk microphysics schemes in atmospheric models and improving climate modeling.</p>",
        "doi": "10.1029/2023ms004028",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth System (JAMES)",
        "publication_date": "2024-07",
        "series_number": "7",
        "volume": "16",
        "issue": "7",
        "pages": "e2023MS004028"
    },
    {
        "id": "authors:cvzmm-fmb67",
        "collection": "authors",
        "collection_id": "cvzmm-fmb67",
        "cite_using_url": "https://authors.library.caltech.edu/records/cvzmm-fmb67",
        "type": "article",
        "title": "Opinion: Optimizing climate models with process knowledge, resolution, and artificial intelligence",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Leung",
                "given_name": "L. Ruby",
                "orcid": "0000-0002-3221-9467"
            },
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "orcid": "0000-0002-7776-2076"
            }
        ],
        "abstract": "<p>Accelerated progress in climate modeling is urgently needed for proactive and effective climate change adaptation. The central challenge lies in accurately representing processes that are small in scale yet climatically important, such as turbulence and cloud formation. These processes will not be explicitly resolvable for the foreseeable future, necessitating the use of parameterizations. We propose a balanced approach that leverages the strengths of traditional process-based parameterizations and contemporary artificial intelligence (AI)-based methods to model subgrid-scale processes. This strategy employs AI to derive data-driven closure functions from both observational and simulated data, integrated within parameterizations that encode system knowledge and conservation laws. In addition, increasing the resolution to resolve a larger fraction of small-scale processes can aid progress toward improved and interpretable climate predictions outside the observed climate distribution. However, currently feasible horizontal resolutions are limited to O(10&thinsp;km) because higher resolutions would impede the creation of the ensembles that are needed for model calibration and uncertainty quantification, for sampling atmospheric and oceanic internal variability, and for broadly exploring and quantifying climate risks. By synergizing decades of scientific development with advanced AI techniques, our approach aims to significantly boost the accuracy, interpretability, and trustworthiness of climate predictions.</p>",
        "doi": "10.5194/acp-24-7041-2024",
        "issn": "1680-7324",
        "publisher": "European Geosciences Union",
        "publication": "Atmospheric Chemistry and Physics",
        "publication_date": "2024-06-19",
        "series_number": "12",
        "volume": "24",
        "issue": "12",
        "pages": "7041-7062"
    },
    {
        "id": "authors:cdg1t-5mm33",
        "collection": "authors",
        "collection_id": "cdg1t-5mm33",
        "cite_using_url": "https://authors.library.caltech.edu/records/cdg1t-5mm33",
        "type": "article",
        "title": "Toward a US Framework for Continuity of Satellite Observations of Earth's Climate and for Supporting Societal Resilience",
        "author": [
            {
                "family_name": "Frankenberg",
                "given_name": "Christian",
                "orcid": "0000-0002-0546-5857",
                "clpid": "Frankenberg-C"
            },
            {
                "family_name": "Michalak",
                "given_name": "Anna M.",
                "orcid": "0000-0002-6152-7979",
                "clpid": "Michalak-Anna-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "literal": "KISS Continuity Study Team"
            }
        ],
        "abstract": "<p>There is growing urgency for improved public and commercial services to support a resilient, secure, and thriving United States (US) in the face of mounting decision\u2010support needs for environmental stewardship and hazard response, as well as for climate change adaptation and mitigation. Sustained space\u2010based Earth observations are critical infrastructure to support the delivery of science and decision\u2010support information with local, national, and global utility. This is reflected in part through the United States' sustained support of a suite of weather and land\u2010imaging satellites. However, outside of these two areas, the US lacks an overarching, systematic plan or framework to identify, prioritize, fund, and implement sustained space\u2010based Earth observations to meet the Nation's full range of needs for science, government policy, and societal support. To aid and accelerate the discussion on our nation's needs, challenges and opportunities associated with sustained critical space\u2010based Earth observations, the Keck Institute for Space Studies (KISS) sponsored a multi\u2010week think\u2010tank study to offer ways forward. Based on this study, the KISS study team suggests the establishment of a robust coordination framework to help address US needs for sustained Earth observations. This coordination framework could account for: (a) approaches to identify and prioritize satellite observations needed to meet US needs for science and services, (b) the rapidly evolving landscape of space\u2010based Earth viewing architecture options and technology improvements with increasing opportunities and lower cost access to space, and (c) the technical and programmatic underpinnings required for proper and comprehensive data stewardship to support a wide range of research and public services.</p>",
        "doi": "10.1029/2023ef003757",
        "issn": "2328-4277",
        "publisher": "American Geophysical Union",
        "publication": "Earth's Future",
        "publication_date": "2024-02",
        "series_number": "2",
        "volume": "12",
        "issue": "2",
        "pages": "e2023EF003757"
    },
    {
        "id": "authors:0677f-qrc81",
        "collection": "authors",
        "collection_id": "0677f-qrc81",
        "cite_using_url": "https://authors.library.caltech.edu/records/0677f-qrc81",
        "type": "article",
        "title": "Accelerating Large-Eddy Simulations of Clouds With Tensor Processing Units",
        "author": [
            {
                "family_name": "Chammas",
                "given_name": "Sheide",
                "orcid": "0000-0001-9001-629X",
                "clpid": "Chammas-Sheide"
            },
            {
                "family_name": "Wang",
                "given_name": "Qing",
                "orcid": "0000-0002-9414-5184",
                "clpid": "Wang-Qing"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Ihme",
                "given_name": "Matthias",
                "orcid": "0000-0002-4158-7050",
                "clpid": "Ihme-Matthias"
            },
            {
                "family_name": "Chen",
                "given_name": "Yi-fan",
                "orcid": "0000-0001-9751-8049",
                "clpid": "Chen-Yi-fan"
            },
            {
                "family_name": "Anderson",
                "given_name": "John",
                "orcid": "0009-0000-5341-8919",
                "clpid": "Anderson-John"
            }
        ],
        "abstract": "<p>Clouds, especially low clouds, are crucial for regulating Earth's energy balance and mediating the response of the climate system to changes in greenhouse gas concentrations. Despite their importance for climate, they remain relatively poorly understood and are inaccurately represented in climate models. A principal reason is that the high computational expense of simulating them with large\u2010eddy simulations (LES) has inhibited broad and systematic numerical experimentation and the generation of large data sets for training parametrization schemes for climate models. Here we demonstrate LES of low clouds on tensor processing units (TPUs), application\u2010specific integrated circuits that were originally developed for machine learning applications. We show that TPUs in conjunction with tailored software implementations can be used to simulate computationally challenging stratocumulus clouds in conditions observed during the Dynamics and Chemistry of Marine Stratocumulus (DYCOMS) field study. The TPU\u2010based LES code successfully reproduces clouds during DYCOMS and opens up the large computational resources available on TPUs to cloud simulations. The code enables unprecedented weak and strong scaling of LES, making it possible, for example, to simulate stratocumulus with 10&times; speedup over real\u2010time evolution in domains with a 34.7 km &times; 53.8 km horizontal cross section. The results open up new avenues for computational experiments and for substantially enlarging the sample of LES available to train parameterizations of low clouds.</p>",
        "doi": "10.1029/2023ms003619",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth System (JAMES)",
        "publication_date": "2023-10",
        "series_number": "10",
        "volume": "15",
        "issue": "10",
        "pages": "e2023MS003619"
    },
    {
        "id": "authors:z0c0r-2jt68",
        "collection": "authors",
        "collection_id": "z0c0r-2jt68",
        "cite_using_url": "https://authors.library.caltech.edu/records/z0c0r-2jt68",
        "type": "article",
        "title": "Harnessing AI and computing to advance climate modelling and prediction",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Behera",
                "given_name": "Swadhin",
                "orcid": "0000-0001-8692-2388",
                "clpid": "Behera-Swadhin"
            },
            {
                "family_name": "Boccaletti",
                "given_name": "Giulio",
                "orcid": "0009-0008-1072-7672",
                "clpid": "Boccaletti-Giulio"
            },
            {
                "family_name": "Deser",
                "given_name": "Clara",
                "orcid": "0000-0002-5517-9103",
                "clpid": "Deser-Clara"
            },
            {
                "family_name": "Emanuel",
                "given_name": "Kerry",
                "orcid": "0000-0002-2066-2082",
                "clpid": "Emanuel-Kerry"
            },
            {
                "family_name": "Ferrari",
                "given_name": "Raffaele",
                "orcid": "0000-0003-1895-4294",
                "clpid": "Ferrari-Raffaele"
            },
            {
                "family_name": "Leung",
                "given_name": "L. Ruby",
                "orcid": "0000-0002-3221-9467",
                "clpid": "Leung-L-Ruby"
            },
            {
                "family_name": "Lin",
                "given_name": "Ning",
                "orcid": "0000-0002-5571-1606",
                "clpid": "Lin-Ning"
            },
            {
                "family_name": "M\u00fcller",
                "given_name": "Thomas",
                "orcid": "0000-0003-1225-1483",
                "clpid": "M\u00fcller-Thomas"
            },
            {
                "family_name": "Navarra",
                "given_name": "Antonio",
                "clpid": "Navarra-Antonio"
            },
            {
                "family_name": "Ndiaye",
                "given_name": "Ousmane",
                "orcid": "0000-0002-5048-4731",
                "clpid": "Ndiaye-Ousmane"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            },
            {
                "family_name": "Tribbia",
                "given_name": "Joseph",
                "orcid": "0000-0003-1639-9688",
                "clpid": "Tribbia-Joseph"
            },
            {
                "family_name": "Yamagata",
                "given_name": "Toshio",
                "orcid": "0000-0003-1267-2149",
                "clpid": "Yamagata-Toshio"
            }
        ],
        "abstract": "<p>There are contrasting views on how to produce the accurate predictions that are needed to guide climate change adaptation. Here, we argue for harnessing artificial intelligence, building on domain-specific knowledge and generating ensembles of moderately high-resolution (10\u201350 km) climate simulations as anchors for detailed hazard models.</p>",
        "doi": "10.1038/s41558-023-01769-3",
        "issn": "1758-678X",
        "publisher": "Nature Publishing Group",
        "publication": "Nature Climate Change",
        "publication_date": "2023-09",
        "series_number": "9",
        "volume": "13",
        "issue": "9",
        "pages": "887-889"
    },
    {
        "id": "authors:8dvrz-1qp80",
        "collection": "authors",
        "collection_id": "8dvrz-1qp80",
        "cite_using_url": "https://authors.library.caltech.edu/records/8dvrz-1qp80",
        "type": "article",
        "title": "Accelerating Scientific Discovery With AI-Aided Automation",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Altintas",
                "given_name": "Ilkay",
                "orcid": "0000-0002-2196-0305"
            },
            {
                "family_name": "Atkins",
                "given_name": "Daniel",
                "orcid": "0000-0001-9002-9613",
                "clpid": "Atkins-Daniel"
            }
        ],
        "abstract": "<div class=\"abstract-text row g-0\">\n<div class=\"col-12\">\n<div class=\"u-mb-1\">\n<div>AI-aided design of experiments and observations, together with robotic instrumentation and automated learning from data, has the potential to transform science and propel it forward with unprecedented speed.</div>\n</div>\n</div>\n</div>",
        "doi": "10.1109/mcse.2024.3352451",
        "issn": "1521-9615",
        "publisher": "IEEE",
        "publication": "Computing in Science & Engineering",
        "publication_date": "2023-09",
        "series_number": "5",
        "volume": "25",
        "issue": "5",
        "pages": "27-30"
    },
    {
        "id": "authors:xhesv-wv708",
        "collection": "authors",
        "collection_id": "xhesv-wv708",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230818-791138000.1",
        "type": "article",
        "title": "The Importance of Hyperspectral Soil Albedo Information for Improving Earth System Model Projections",
        "author": [
            {
                "family_name": "Braghiere",
                "given_name": "R. K.",
                "orcid": "0000-0002-7722-717X",
                "clpid": "Kerches-Braghiere-Renato"
            },
            {
                "family_name": "Wang",
                "given_name": "Y.",
                "orcid": "0000-0002-3729-2743",
                "clpid": "Wang-Yujie"
            },
            {
                "family_name": "Gagn\u00e9\u2010Landmann",
                "given_name": "A.",
                "clpid": "Gagn\u00e9\u2010Landmann-A"
            },
            {
                "family_name": "Brodrick",
                "given_name": "P. G.",
                "orcid": "0000-0001-9497-7661",
                "clpid": "Brodrick-Philip-G"
            },
            {
                "family_name": "Bloom",
                "given_name": "A. A.",
                "orcid": "0000-0002-1486-1499",
                "clpid": "Bloom-A-Anthony"
            },
            {
                "family_name": "Norton",
                "given_name": "A. J.",
                "orcid": "0000-0001-7708-3914",
                "clpid": "Norton-Alexander-J"
            },
            {
                "family_name": "Ma",
                "given_name": "S.",
                "orcid": "0000-0002-6494-724X",
                "clpid": "Ma-Shuang"
            },
            {
                "family_name": "Levine",
                "given_name": "P.",
                "orcid": "0000-0002-1248-6920",
                "clpid": "Levvine-Paul"
            },
            {
                "family_name": "Longo",
                "given_name": "M.",
                "orcid": "0000-0001-5062-6245",
                "clpid": "Longo-Marcos"
            },
            {
                "family_name": "Deck",
                "given_name": "K.",
                "clpid": "Deck-Katherine-M"
            },
            {
                "family_name": "Gentine",
                "given_name": "P.",
                "orcid": "0000-0002-0845-8345",
                "clpid": "Gentine-Pierre"
            },
            {
                "family_name": "Worden",
                "given_name": "J. R.",
                "orcid": "0000-0003-0257-9549",
                "clpid": "Worden-John-R"
            },
            {
                "family_name": "Frankenberg",
                "given_name": "C.",
                "orcid": "0000-0002-0546-5857",
                "clpid": "Frankenberg-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "AbstractEarth system models (ESMs) typically simplify the representation of land surface spectral albedo to two values, which correspond to the photosynthetically active radiation (PAR, 400\u2013700\u00a0nm) and the near infrared (NIR, 700\u20132,500\u00a0nm) spectral bands. However, the availability of hyperspectral observations now allows for a more direct retrieval of ecological parameters and reduction of uncertainty in surface reflectance. To investigate sensitivity and quantify biases of incorporating hyperspectral albedo information into ESMs, we examine how shortwave soil albedo affects surface radiative forcing and simulations of the carbon and water cycles. Results reveal that the use of two broadband values to represent soil albedo can introduce systematic radiative\u2010forcing differences compared to a hyperspectral representation. Specifically, we estimate soil albedo biases of \u00b10.2 over desert areas, which can result in spectrally integrated radiative forcing divergences of up to 30\u00a0W\u00a0m\u207b\u00b2, primarily due to discrepancies in the blue (404\u2013504\u00a0nm) and far\u2010red (702\u2013747\u00a0nm) regions. Furthermore, coupled land\u2010atmosphere simulations indicate a significant difference in net solar flux at the top of the atmosphere (&gt;3.3\u00a0W\u00a0m\u207b\u00b2), which can impact global energy fluxes, rainfall, temperature, and photosynthesis. Finally, simulations show that considering the hyperspectrally resolved soil reflectance leads to increased maximum daily temperatures under current and future CO\u2082 concentrations.",
        "doi": "10.1029/2023av000910",
        "issn": "2576-604X",
        "publisher": "American Geophysical Union",
        "publication": "AGU Advances",
        "publication_date": "2023-08",
        "series_number": "4",
        "volume": "4",
        "issue": "4",
        "pages": "Art. No. e2023AV000910"
    },
    {
        "id": "authors:67c6a-8pm34",
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        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230719-853635200.6",
        "type": "article",
        "title": "Thank You to Our 2022 Peer Reviewers",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X",
                "clpid": "Griffies-Stephen-M"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391",
                "clpid": "Fan-Jiwen"
            },
            {
                "family_name": "MacBean",
                "given_name": "Natasha",
                "orcid": "0000-0001-6797-4836",
                "clpid": "MacBean-Natasha"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The editors of Journal of Advances in Modeling Earth Systems thank the 702 reviewers who provided 1362 reviews during 2022. Their hard work and insights, typically done anonymously, benefits authors, readers, and the broader science community.",
        "doi": "10.1029/2023ms003785",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2023-05",
        "series_number": "5",
        "volume": "15",
        "issue": "5",
        "pages": "Art. No. e2023MS003785"
    },
    {
        "id": "authors:xzbew-dbe85",
        "collection": "authors",
        "collection_id": "xzbew-dbe85",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230714-263898400.4",
        "type": "article",
        "title": "The Flux\u2010Differencing Discontinuous Galerkin Method Applied to an Idealized Fully Compressible Nonhydrostatic Dry Atmosphere",
        "author": [
            {
                "family_name": "Souza",
                "given_name": "A. N.",
                "orcid": "0000-0001-8025-3558",
                "clpid": "Souza-Andre-N"
            },
            {
                "family_name": "He",
                "given_name": "J.",
                "clpid": "He-Jia"
            },
            {
                "family_name": "Bischoff",
                "given_name": "T.",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Waruszewski",
                "given_name": "M.",
                "orcid": "0009-0001-8918-4314",
                "clpid": "Waruszewski-Maciej"
            },
            {
                "family_name": "Novak",
                "given_name": "L.",
                "orcid": "0000-0002-2863-5601",
                "clpid": "Novak-Lenka"
            },
            {
                "family_name": "Barra",
                "given_name": "V.",
                "orcid": "0000-0003-1129-2056",
                "clpid": "Barra-Valeria"
            },
            {
                "family_name": "Gibson",
                "given_name": "T.",
                "clpid": "Gibson-T"
            },
            {
                "family_name": "Sridhar",
                "given_name": "A.",
                "orcid": "0000-0002-2642-8246",
                "clpid": "Sridhar-Akshay"
            },
            {
                "family_name": "Kandala",
                "given_name": "S.",
                "orcid": "0000-0002-6790-1597",
                "clpid": "Kandala-Sriharsha"
            },
            {
                "family_name": "Byrne",
                "given_name": "S.",
                "orcid": "0000-0002-5466-3112",
                "clpid": "Byrne-Simon"
            },
            {
                "family_name": "Wilcox",
                "given_name": "L. C.",
                "clpid": "Wilcox-Lucas-C"
            },
            {
                "family_name": "Kozdon",
                "given_name": "J.",
                "orcid": "0000-0002-2493-4292",
                "clpid": "Kozdon-Jeremy-E"
            },
            {
                "family_name": "Giraldo",
                "given_name": "F. X.",
                "orcid": "0000-0001-8965-1202",
                "clpid": "Giraldo-Francis-X"
            },
            {
                "family_name": "Knoth",
                "given_name": "O.",
                "orcid": "0000-0002-1003-3207",
                "clpid": "Knoth-Oswald"
            },
            {
                "family_name": "Marshall",
                "given_name": "J.",
                "clpid": "Marshall-J"
            },
            {
                "family_name": "Ferrari",
                "given_name": "R.",
                "orcid": "0000-0003-1895-4294",
                "clpid": "Ferrari-Raffaele"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Dynamical cores used to study the circulation of the atmosphere employ various numerical methods ranging from finite-volume, spectral element, global spectral, and hybrid methods. In this work, we explore the use of Flux-Differencing Discontinuous Galerkin (FDDG) methods to simulate a fully compressible dry atmosphere at various resolutions. We show that the method offers a judicious compromise between high-order accuracy and stability for large-eddy simulations and simulations of the atmospheric general circulation. In particular, filters, divergence damping, diffusion, hyperdiffusion, or sponge-layers are not required to ensure stability; only the numerical dissipation naturally afforded by FDDG is necessary. We apply the method to the simulation of dry convection in an atmospheric boundary layer and in a global atmospheric dynamical core in the standard benchmark of Held and Suarez (1994, https://doi.org/10.1175/1520-0477(1994)075\u30081825:apftio\u30092.0.co;2).",
        "doi": "10.1029/2022ms003527",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2023-04",
        "series_number": "4",
        "volume": "15",
        "issue": "4",
        "pages": "Art. No. e2022MS003527"
    },
    {
        "id": "authors:8377w-q8k46",
        "collection": "authors",
        "collection_id": "8377w-q8k46",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230627-116746000.8",
        "type": "article",
        "title": "The Flux-Differencing Discontinuous Galerkin Method Applied to an Idealized Fully Compressible Nonhydrostatic Dry Atmosphere",
        "author": [
            {
                "family_name": "Souza",
                "given_name": "A. N.",
                "orcid": "0000-0001-8025-3558",
                "clpid": "Souza-Andre-N"
            },
            {
                "family_name": "He",
                "given_name": "J.",
                "clpid": "He-Jia"
            },
            {
                "family_name": "Bischoff",
                "given_name": "T.",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Waruszewski",
                "given_name": "M.",
                "orcid": "0009-0001-8918-4314",
                "clpid": "Waruszewski-Maciej"
            },
            {
                "family_name": "Novak",
                "given_name": "L.",
                "orcid": "0000-0002-2863-5601",
                "clpid": "Novak-Lenka"
            },
            {
                "family_name": "Barra",
                "given_name": "V.",
                "orcid": "0000-0003-1129-2056",
                "clpid": "Barra-Valeria"
            },
            {
                "family_name": "Gibson",
                "given_name": "T.",
                "clpid": "Gibson-T"
            },
            {
                "family_name": "Sridhar",
                "given_name": "A.",
                "orcid": "0000-0002-2642-8246",
                "clpid": "Sridhar-Akshay"
            },
            {
                "family_name": "Kandala",
                "given_name": "S.",
                "orcid": "0000-0002-6790-1597",
                "clpid": "Kandala-Sriharsha"
            },
            {
                "family_name": "Byrne",
                "given_name": "S.",
                "orcid": "0000-0002-5466-3112",
                "clpid": "Byrne-Simon"
            },
            {
                "family_name": "Wilcox",
                "given_name": "L. C.",
                "clpid": "Wilcox-Lucas-C"
            },
            {
                "family_name": "Kozdon",
                "given_name": "J.",
                "orcid": "0000-0002-2493-4292",
                "clpid": "Kozdon-Jeremy-E"
            },
            {
                "family_name": "Giraldo",
                "given_name": "F. X.",
                "orcid": "0000-0001-8965-1202",
                "clpid": "Giraldo-Francis-X"
            },
            {
                "family_name": "Knoth",
                "given_name": "O.",
                "orcid": "0000-0002-1003-3207",
                "clpid": "Knoth-Oswald"
            },
            {
                "family_name": "Marshall",
                "given_name": "J.",
                "clpid": "Marshall-John"
            },
            {
                "family_name": "Ferrari",
                "given_name": "R.",
                "orcid": "0000-0003-1895-4294",
                "clpid": "Ferrari-Raffaele"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Dynamical cores used to study the circulation of the atmosphere employ various numerical methods ranging from finite-volume, spectral element, global spectral, and hybrid methods. In this work, we explore the use of Flux-Differencing Discontinuous Galerkin (FDDG) methods to simulate a fully compressible dry atmosphere at various resolutions. We show that the method offers a judicious compromise between high-order accuracy and stability for large-eddy simulations and simulations of the atmospheric general circulation. In particular, filters, divergence damping, diffusion, hyperdiffusion, or sponge-layers are not required to ensure stability; only the numerical dissipation naturally afforded by FDDG is necessary. We apply the method to the simulation of dry convection in an atmospheric boundary layer and in a global atmospheric dynamical core in the standard benchmark of Held and Suarez (1994, https://doi.org/10.1175/1520-0477(1994)075\u30081825:apftio\u30092.0.co;2).",
        "doi": "10.1029/2022ms003527",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2023-04",
        "series_number": "4",
        "volume": "15",
        "issue": "4",
        "pages": "Art. No. e2022MS003527"
    },
    {
        "id": "authors:sj7hg-0bc07",
        "collection": "authors",
        "collection_id": "sj7hg-0bc07",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230509-291707400.5",
        "type": "article",
        "title": "Aims and Scope of JAMES",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X",
                "clpid": "Griffies-Stephen-M"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391",
                "clpid": "Fan-Jiwen"
            },
            {
                "family_name": "MacBean",
                "given_name": "Natasha",
                "orcid": "0000-0001-6797-4836",
                "clpid": "MacBean-Natasha"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The mission of AGU's Journal of Advances in Modeling Earth Systems (JAMES) is to publish original research papers that advance the science underlying Earth system models and emerging from their use. JAMES' scope encompasses the outer envelope of the Earth system including the atmosphere, oceans, land surface, and cryosphere. It publishes papers that expand capabilities to model, understand, and predict the Earth system and the physical, chemical, and biological processes shaping it. In this editorial, we present general principles as well as specific notions that guide the strategy of JAMES' editors in realizing the journal's mission. This document serves as an update to Griffies et al. (2021), https://doi.org/10.1029/2021MS002567.",
        "doi": "10.1029/2023ms003741",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2023-04",
        "series_number": "4",
        "volume": "15",
        "issue": "4",
        "pages": "Art. No. e2023MS003741"
    },
    {
        "id": "authors:r1xdb-d5582",
        "collection": "authors",
        "collection_id": "r1xdb-d5582",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20230705-476466000.31",
        "type": "article",
        "title": "Aims and Scope of JAMES",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X",
                "clpid": "Griffies-Stephen-M"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391",
                "clpid": "Fan-Jiwen"
            },
            {
                "family_name": "MacBean",
                "given_name": "Natasha",
                "orcid": "0000-0001-6797-4836",
                "clpid": "MacBean-Natasha"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The mission of AGU's Journal of Advances in Modeling Earth Systems (JAMES) is to publish original research papers that advance the science underlying Earth system models and emerging from their use. JAMES' scope encompasses the outer envelope of the Earth system including the atmosphere, oceans, land surface, and cryosphere. It publishes papers that expand capabilities to model, understand, and predict the Earth system and the physical, chemical, and biological processes shaping it. In this editorial, we present general principles as well as specific notions that guide the strategy of JAMES' editors in realizing the journal's mission. This document serves as an update to Griffies et al. (2021), https://doi.org/10.1029/2021MS002567.",
        "doi": "10.1029/2023ms003741",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2023-04",
        "series_number": "4",
        "volume": "15",
        "issue": "4",
        "pages": "Art. No. e2023MS003741"
    },
    {
        "id": "authors:qafpz-pzq58",
        "collection": "authors",
        "collection_id": "qafpz-pzq58",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20221013-45138000.1",
        "type": "article",
        "title": "Ensemble Kalman inversion for sparse learning of dynamical systems from time-averaged data",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew M.",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            },
            {
                "family_name": "Wu",
                "given_name": "Jin-Long",
                "clpid": "Wu-Jin-Long"
            }
        ],
        "abstract": "Enforcing sparse structure within learning has led to significant advances in the field of data-driven discovery of dynamical systems. However, such methods require access not only to timeseries of the state of the dynamical system, but also to the time derivative. In many applications, the data are available only in the form of time-averages such as moments and autocorrelation functions. We propose a sparse learning methodology to discover the vector fields defining a (possibly stochastic or partial) differential equation, using only time-averaged statistics. Such a formulation of sparse learning naturally leads to a nonlinear inverse problem to which we apply the methodology of ensemble Kalman inversion (EKI). EKI is chosen because it may be formulated in terms of the iterative solution of quadratic optimization problems; sparsity is then easily imposed. We then apply the EKI-based sparse learning methodology to various examples governed by stochastic differential equations (a noisy Lorenz 63 system), ordinary differential equations (Lorenz 96 system and coalescence equations), and a partial differential equation (the Kuramoto-Sivashinsky equation). The results demonstrate that time-averaged statistics can be used for data-driven discovery of differential equations using sparse EKI. The proposed sparse learning methodology extends the scope of data-driven discovery of differential equations to previously challenging applications and data-acquisition scenarios.",
        "doi": "10.1016/j.jcp.2022.111559",
        "issn": "0021-9991",
        "publisher": "Elsevier",
        "publication": "Journal of Computational Physics",
        "publication_date": "2022-12-01",
        "volume": "470",
        "pages": "Art. No. 111559"
    },
    {
        "id": "authors:sdv6s-rr183",
        "collection": "authors",
        "collection_id": "sdv6s-rr183",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20220926-576391900.2",
        "type": "article",
        "title": "Ensemble-Based Experimental Design for Targeting Data Acquisition to Inform Climate Models",
        "author": [
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Howland",
                "given_name": "Michael F.",
                "orcid": "0000-0002-2878-3874",
                "clpid": "Howland-Michael-F"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew M.",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            }
        ],
        "abstract": "Data required to calibrate uncertain general circulation model (GCM) parameterizations are often only available in limited regions or time periods, for example, observational data from field campaigns, or data generated in local high-resolution simulations. This raises the question of where and when to acquire additional data to be maximally informative about parameterizations in a GCM. Here we construct a new ensemble-based parallel algorithm to automatically target data acquisition to regions and times that maximize the uncertainty reduction, or information gain, about GCM parameters. The algorithm uses a Bayesian framework that exploits a quantified distribution of GCM parameters as a measure of uncertainty. This distribution is informed by time-averaged climate statistics restricted to local regions and times. The algorithm is embedded in the recently developed calibrate-emulate-sample framework, which performs efficient model calibration and uncertainty quantification with only O(10\u00b2) model evaluations, compared with O(10\u2075) evaluations typically needed for traditional approaches to Bayesian calibration. We demonstrate the algorithm with an idealized GCM, with which we generate surrogates of local data. In this perfect-model setting, we calibrate parameters and quantify uncertainties in a quasi-equilibrium convection scheme in the GCM. We consider targeted data that are (a) localized in space for statistically stationary simulations, and (b) localized in space and time for seasonally varying simulations. In these proof-of-concept applications, the calculated information gain reflects the reduction in parametric uncertainty obtained from Bayesian inference when harnessing a targeted sample of data. The largest information gain typically, but not always, results from regions near the intertropical convergence zone.",
        "doi": "10.1029/2022ms002997",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2022-09",
        "series_number": "9",
        "volume": "14",
        "issue": "9",
        "pages": "Art. No. e2022MS002997"
    },
    {
        "id": "authors:nj6wn-jwq16",
        "collection": "authors",
        "collection_id": "nj6wn-jwq16",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210719-210149563",
        "type": "article",
        "title": "Iterated Kalman methodology for inverse problems",
        "author": [
            {
                "family_name": "Huang",
                "given_name": "Daniel Zhengyu",
                "clpid": "Huang-Zhengyu-Daniel"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew M.",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            }
        ],
        "abstract": "This paper is focused on the optimization approach to the solution of inverse problems. We introduce a stochastic dynamical system in which the parameter-to-data map is embedded, with the goal of employing techniques from nonlinear Kalman filtering to estimate the parameter given the data. The extended Kalman filter (which we refer to as ExKI in the context of inverse problems) can be effective for some inverse problems approached this way, but is impractical when the forward map is not readily differentiable and is given as a black box, and also for high dimensional parameter spaces because of the need to propagate large covariance matrices. Application of ensemble Kalman filters, for example use of the ensemble Kalman inversion (EKI) algorithm, has emerged as a useful tool which overcomes both of these issues: it is derivative free and works with a low-rank covariance approximation formed from the ensemble. In this paper, we work with the ExKI, EKI, and a variant on EKI which we term unscented Kalman inversion (UKI).\n\nThe paper contains two main contributions. Firstly, we identify a novel stochastic dynamical system in which the parameter-to-data map is embedded. We present theory in the linear case to show exponential convergence of the mean of the filtering distribution to the solution of a regularized least squares problem. This is in contrast to previous work in which the EKI has been employed where the dynamical system used leads to algebraic convergence to an unregularized problem. Secondly, we show that the application of the UKI to this novel stochastic dynamical system yields improved inversion results, in comparison with the application of EKI to the same novel stochastic dynamical system.\n\nThe numerical experiments include proof-of-concept linear examples and various applied nonlinear inverse problems: learning of permeability parameters in subsurface flow; learning the damage field from structure deformation; learning the Navier-Stokes initial condition from solution data at positive times; learning subgrid-scale parameters in a general circulation model (GCM) from time-averaged statistics.",
        "doi": "10.1016/j.jcp.2022.111262",
        "issn": "0021-9991",
        "publisher": "Elsevier",
        "publication": "Journal of Computational Physics",
        "publication_date": "2022-08-15",
        "volume": "463",
        "pages": "Art. No. 111262"
    },
    {
        "id": "authors:f2xnx-h3a43",
        "collection": "authors",
        "collection_id": "f2xnx-h3a43",
        "cite_using_url": "https://authors.library.caltech.edu/records/f2xnx-h3a43",
        "type": "article",
        "title": "Large-eddy simulations with ClimateMachine v0.2.0: a new open-source code for atmospheric simulations on GPUs and CPUs",
        "author": [
            {
                "family_name": "Sridhar",
                "given_name": "Akshay",
                "orcid": "0000-0002-2642-8246",
                "clpid": "Sridhar-Akshay"
            },
            {
                "family_name": "Tissaoui",
                "given_name": "Yassine",
                "orcid": "0000-0001-6676-2233"
            },
            {
                "family_name": "Marras",
                "given_name": "Simone",
                "orcid": "0000-0002-7498-049X"
            },
            {
                "family_name": "Shen",
                "given_name": "Zhaoyi",
                "orcid": "0000-0002-0444-4720",
                "clpid": "Shen-Zhaoyi"
            },
            {
                "family_name": "Kawczynski",
                "given_name": "Charles",
                "clpid": "Kawczynski-Charles"
            },
            {
                "family_name": "Byrne",
                "given_name": "Simon",
                "orcid": "0000-0001-8048-6810",
                "clpid": "Byrne-Simon"
            },
            {
                "family_name": "Pamnany",
                "given_name": "Kiran",
                "orcid": "0009-0009-2340-3658",
                "clpid": "Pamnany-Kiran"
            },
            {
                "family_name": "Waruszewski",
                "given_name": "Maciej",
                "orcid": "0009-0001-8918-4314"
            },
            {
                "family_name": "Gibson",
                "given_name": "Thomas H.",
                "orcid": "0000-0002-7978-6848"
            },
            {
                "family_name": "Kozdon",
                "given_name": "Jeremy E.",
                "orcid": "0000-0002-2493-4292"
            },
            {
                "family_name": "Churavy",
                "given_name": "Valentin",
                "orcid": "0000-0002-9033-165X"
            },
            {
                "family_name": "Wilcox",
                "given_name": "Lucas C."
            },
            {
                "family_name": "Giraldo",
                "given_name": "Francis X.",
                "orcid": "0000-0001-8965-1202"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<p>We introduce ClimateMachine, a new open-source atmosphere modeling framework which uses the Julia language and is designed to be scalable on central processing units (CPUs) and graphics processing units (GPUs). ClimateMachine uses a common framework both for coarser-resolution global simulations and for high-resolution, limited-area large-eddy simulations (LESs). Here, we demonstrate the LES configuration of the atmosphere model in canonical benchmark cases and atmospheric flows using a total energy-conserving nodal discontinuous Galerkin (DG) discretization of the governing equations. Resolution dependence, conservation characteristics, and scaling metrics are examined in comparison with existing LES codes. They demonstrate the utility of ClimateMachine as a modeling tool for limited-area LES flow configurations.</p>",
        "doi": "10.5194/gmd-15-6259-2022",
        "issn": "1991-9603",
        "publisher": "European Geosciences Union",
        "publication": "Geoscientific Model Development",
        "publication_date": "2022-08-12",
        "series_number": "15",
        "volume": "15",
        "issue": "15",
        "pages": "6259-6284"
    },
    {
        "id": "authors:1q6gn-mvc46",
        "collection": "authors",
        "collection_id": "1q6gn-mvc46",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20220810-402975000",
        "type": "article",
        "title": "Training physics\u2010based machine\u2010learning parameterizations with gradient\u2010free ensemble Kalman methods",
        "author": [
            {
                "family_name": "Lopez-Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895",
                "clpid": "Lopez-Gomez-Ignacio"
            },
            {
                "family_name": "Christopoulos",
                "given_name": "Costa",
                "orcid": "0000-0002-8552-465X",
                "clpid": "Christopoulos-Costa-D"
            },
            {
                "family_name": "Ervik",
                "given_name": "Haakon Ludvig Langeland",
                "orcid": "0000-0003-2912-5774",
                "clpid": "Ervik-Haakon-Ludvig-Langeland"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Cohen",
                "given_name": "Yair",
                "orcid": "0000-0002-9615-2476",
                "clpid": "Cohen-Yair"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Most machine learning applications in Earth system modeling currently rely on gradient-based supervised learning. This imposes stringent constraints on the nature of the data used for training (typically, residual time tendencies are needed), and it complicates learning about the interactions between machine-learned parameterizations and other components of an Earth system model. Approaching learning about process-based parameterizations as an inverse problem resolves many of these issues, since it allows parameterizations to be trained with partial observations or statistics that directly relate to quantities of interest in long-term climate projections. Here we demonstrate the effectiveness of Kalman inversion methods in treating learning about parameterizations as an inverse problem. We consider two different algorithms: unscented and ensemble Kalman inversion. Both methods involve highly parallelizable forward model evaluations, converge exponentially fast, and do not require gradient computations. In addition, unscented Kalman inversion provides a measure of parameter uncertainty. We illustrate how training parameterizations can be posed as a regularized inverse problem and solved by ensemble Kalman methods through the calibration of an eddy-diffusivity mass-flux scheme for subgrid-scale turbulence and convection, using data generated by large-eddy simulations. We find the algorithms amenable to batching strategies, robust to noise and model failures, and efficient in the calibration of hybrid parameterizations that can include empirical closures and neural networks.",
        "doi": "10.1029/2022ms003105",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2022-08-11",
        "pages": "Art. No. e2022MS003105"
    },
    {
        "id": "authors:s3q2y-tpm38",
        "collection": "authors",
        "collection_id": "s3q2y-tpm38",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20220815-504980000",
        "type": "article",
        "title": "An Efficient Bayesian Approach to Learning Droplet Collision Kernels: Proof of Concept Using \"Cloudy,\" a New n-Moment Bulk Microphysics Scheme",
        "author": [
            {
                "family_name": "Bieli",
                "given_name": "Melanie",
                "orcid": "0000-0002-2056-9486",
                "clpid": "Bieli-Melanie"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "De Jong",
                "given_name": "Emily K.",
                "orcid": "0000-0002-5310-4554",
                "clpid": "De-Jong-Emily-K"
            },
            {
                "family_name": "Jaruga",
                "given_name": "Anna",
                "orcid": "0000-0003-3194-6440",
                "clpid": "Jaruga-Anna"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            }
        ],
        "abstract": "The small-scale microphysical processes governing the formation of precipitation particles cannot be resolved explicitly by cloud resolving and climate models. Instead, they are represented by microphysics schemes that are based on a combination of theoretical knowledge, statistical assumptions, and fitting to data (\"tuning\"). Historically, tuning was done in an ad hoc fashion, leading to parameter choices that are not explainable or repeatable. Recent work has treated it as an inverse problem that can be solved by Bayesian inference. The posterior distribution of the parameters given the data\u2014the solution of Bayesian inference\u2014is found through computationally expensive sampling methods, which require over O(10\u2075) evaluations of the forward model; this is prohibitive for many models. We present a proof of concept of Bayesian learning applied to a new bulk microphysics scheme named \"Cloudy,\" using the recently developed Calibrate-Emulate-Sample (CES) algorithm. Cloudy models collision-coalescence and collisional breakup of cloud droplets with an adjustable number of prognostic moments and with easily modifiable assumptions for the cloud droplet mass distribution and the collision kernel. The CES algorithm uses machine learning tools to accelerate Bayesian inference by reducing the number of forward evaluations needed to O(10\u00b2). It also exhibits a smoothing effect when forward evaluations are polluted by noise. In a suite of perfect-model experiments, we show that CES enables computationally efficient Bayesian inference of parameters in Cloudy from noisy observations of moments of the droplet mass distribution. In an additional imperfect-model experiment, a collision kernel parameter is successfully learned from output generated by a Lagrangian particle-based microphysics model.",
        "doi": "10.1029/2022ms002994",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2022-08",
        "series_number": "8",
        "volume": "14",
        "issue": "8",
        "pages": "Art. No. e2022MS002994"
    },
    {
        "id": "authors:4xm8c-sh061",
        "collection": "authors",
        "collection_id": "4xm8c-sh061",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20220325-220336231",
        "type": "article",
        "title": "Epidemic management and control through risk-dependent individual contact interventions",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Wu",
                "given_name": "Jinlong",
                "orcid": "0000-0001-7438-4228",
                "clpid": "Wu-Jinlong"
            },
            {
                "family_name": "B\u00f6ttcher",
                "given_name": "Lucas",
                "orcid": "0000-0003-1700-1897",
                "clpid": "B\u00f6ttcher-Lucas"
            },
            {
                "family_name": "Burov",
                "given_name": "Dmitry",
                "orcid": "0000-0002-5060-6794",
                "clpid": "Burov-Dmitry"
            },
            {
                "family_name": "Garbuno-I\u00f1igo",
                "given_name": "Alfredo",
                "orcid": "0000-0003-3279-619X",
                "clpid": "Garbuno-I\u00f1igo-Alfredo"
            },
            {
                "family_name": "Wagner",
                "given_name": "Gregory L.",
                "orcid": "0000-0001-5317-2445",
                "clpid": "Wagner-Gregory-L"
            },
            {
                "family_name": "Pei",
                "given_name": "Sen",
                "orcid": "0000-0002-7072-2995",
                "clpid": "Pei-Sen"
            },
            {
                "family_name": "Daraio",
                "given_name": "Chiara",
                "orcid": "0000-0001-5296-4440",
                "clpid": "Daraio-C"
            },
            {
                "family_name": "Ferrari",
                "given_name": "Raffaele",
                "orcid": "0000-0003-1895-4294",
                "clpid": "Ferrari-Raffaele"
            },
            {
                "family_name": "Shaman",
                "given_name": "Jeffrey",
                "orcid": "0000-0002-7216-7809",
                "clpid": "Shaman-Jeffrey"
            }
        ],
        "abstract": "Testing, contact tracing, and isolation (TTI) is an epidemic management and control approach that is difficult to implement at scale because it relies on manual tracing of contacts. Exposure notification apps have been developed to digitally scale up TTI by harnessing contact data obtained from mobile devices; however, exposure notification apps provide users only with limited binary information when they have been directly exposed to a known infection source. Here we demonstrate a scalable improvement to TTI and exposure notification apps that uses data assimilation (DA) on a contact network. Network DA exploits diverse sources of health data together with the proximity data from mobile devices that exposure notification apps rely upon. It provides users with continuously assessed individual risks of exposure and infection, which can form the basis for targeting individual contact interventions. Simulations of the early COVID-19 epidemic in New York City are used to establish proof-of-concept. In the simulations, network DA identifies up to a factor 2 more infections than contact tracing when both harness the same contact data and diagnostic test data. This remains true even when only a relatively small fraction of the population uses network DA. When a sufficiently large fraction of the population (\u2273 75%) uses network DA and complies with individual contact interventions, targeting contact interventions with network DA reduces deaths by up to a factor 4 relative to TTI. Network DA can be implemented by expanding the computational backend of existing exposure notification apps, thus greatly enhancing their capabilities. Implemented at scale, it has the potential to precisely and effectively control future epidemics while minimizing economic disruption.",
        "doi": "10.1371/journal.pcbi.1010171",
        "pmcid": "PMC9223336",
        "issn": "1553-734X",
        "publisher": "Public Library of Science",
        "publication": "PLoS Computational Biology",
        "publication_date": "2022-06-23",
        "series_number": "6",
        "volume": "18",
        "issue": "6",
        "pages": "Art. No. e1010171"
    },
    {
        "id": "authors:pfx6k-bp417",
        "collection": "authors",
        "collection_id": "pfx6k-bp417",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20220609-798289200",
        "type": "article",
        "title": "Thank You to Our 2021 Reviewers",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X",
                "clpid": "Griffies-Stephen-M"
            },
            {
                "family_name": "Blyth",
                "given_name": "Eleanor Mary",
                "orcid": "0000-0002-5052-238X",
                "clpid": "Blyth-Eleanor-Mary"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391",
                "clpid": "Fan-Jiwen"
            },
            {
                "family_name": "MacBean",
                "given_name": "Natasha",
                "orcid": "0000-0001-6797-4836",
                "clpid": "MacBean-Natasha"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "As the editors of a scientific journal, we have the honor of front-row seats to the peer review process. We watch as reviewers bring fresh and frank perspectives to authors' work, identifying weakness in conception or expression, suggesting refinements, and urging authors to clarify a point or to better support an argument. The process is occasionally uncomfortable but almost always respectful, constructive, and productive. The final papers are uniformly better for this input, thus exemplifying the power of collaboration in the scientific process. At the Journal of Advances in Modeling Earth Systems (JAMES), we are fortunate to have a pool of reviewers who volunteer their time, knowledge, and intelligence to improve the work of their colleagues and peers. It is no small task: In 2021, we received 1,088 reviews by 689 individuals. Speaking for ourselves as editors, the 43 devoted associate editors, and the 696 authors, we thank each of you for your selfless contributions to strengthening our community.\n\nThe editors of Journal of Advances in Modeling Earth Systems thank the 689 reviewers who provided 1,088 reviews during 2021. Their hard work and insights, typically done anonymously, benefits authors, readers, and the broader science community.",
        "doi": "10.1029/2022ms003133",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2022-04",
        "series_number": "4",
        "volume": "14",
        "issue": "4",
        "pages": "Art. No. e2022MS003133"
    },
    {
        "id": "authors:by16d-5rc82",
        "collection": "authors",
        "collection_id": "by16d-5rc82",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210528-094924009",
        "type": "article",
        "title": "A Library of Large-Eddy Simulations Forced by Global Climate Models",
        "author": [
            {
                "family_name": "Shen",
                "given_name": "Zhaoyi",
                "orcid": "0000-0002-0444-4720",
                "clpid": "Shen-Zhaoyi"
            },
            {
                "family_name": "Sridhar",
                "given_name": "Akshay",
                "orcid": "0000-0002-2642-8246",
                "clpid": "Sridhar-Akshay"
            },
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Jaruga",
                "given_name": "Anna",
                "orcid": "0000-0003-3194-6440",
                "clpid": "Jaruga-Anna"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Advances in high-performance computing have enabled large-eddy simulations (LES) of turbulence, convection, and clouds. However, their potential to improve parameterizations in global climate models (GCMs) is only beginning to be harnessed, with relatively few canonical LES available so far. The purpose of this paper is to begin creating a public LES library that expands the training data available for calibrating and evaluating GCM parameterizations. To do so, we use an experimental setup in which LES are driven by large-scale forcings from GCMs, which in principle can be used at any location, any time of year, and in any climate state. We use this setup to create a library of LES of clouds across the tropics and subtropics, in the present and in a warmer climate, with a focus on the transition from stratocumulus to shallow cumulus over the East Pacific. The LES results are relatively insensitive to the choice of host GCM driving the LES. Driven with large-scale forcing under global warming, the LES simulate a positive but weak shortwave cloud feedback, adding to the accumulating evidence that low clouds amplify global warming.",
        "doi": "10.1029/2021MS002631",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modelling Earth Systems",
        "publication_date": "2022-03",
        "series_number": "3",
        "volume": "14",
        "issue": "3",
        "pages": "Art. No. e2021MS002631"
    },
    {
        "id": "authors:w8jdm-e8b55",
        "collection": "authors",
        "collection_id": "w8jdm-e8b55",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210823-173258629",
        "type": "article",
        "title": "Parameter Uncertainty Quantification in an Idealized GCM With a Seasonal Cycle",
        "author": [
            {
                "family_name": "Howland",
                "given_name": "Michael F.",
                "orcid": "0000-0002-2878-3874",
                "clpid": "Howland-Michael-F"
            },
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Climate models are generally calibrated manually by comparing selected climate statistics, such as the global top-of-atmosphere energy balance, to observations. The manual tuning only targets a limited subset of observational data and parameters. Bayesian calibration can estimate climate model parameters and their uncertainty using a larger fraction of the available data and automatically exploring the parameter space more broadly. In Bayesian learning, it is natural to exploit the seasonal cycle, which has large amplitude compared with anthropogenic climate change in many climate statistics. In this study, we develop methods for the calibration and uncertainty quantification (UQ) of model parameters exploiting the seasonal cycle, and we demonstrate a proof-of-concept with an idealized general circulation model (GCM). UQ is performed using the calibrate-emulate-sample approach, which combines stochastic optimization and machine learning emulation to speed up Bayesian learning. The methods are demonstrated in a perfect-model setting through the calibration and UQ of a convective parameterization in an idealized GCM with a seasonal cycle. Calibration and UQ based on seasonally averaged climate statistics, compared to annually averaged, reduces the calibration error by up to an order of magnitude and narrows the spread of the non-Gaussian posterior distributions by factors between two and five, depending on the variables used for UQ. The reduction in the spread of the parameter posterior distribution leads to a reduction in the uncertainty of climate model predictions.",
        "doi": "10.1029/2021MS002735",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modelling Earth Systems",
        "publication_date": "2022-03",
        "series_number": "3",
        "volume": "14",
        "issue": "3",
        "pages": "Art. No. e2021MS002735"
    },
    {
        "id": "authors:pjjee-1w296",
        "collection": "authors",
        "collection_id": "pjjee-1w296",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20201027-125955966",
        "type": "article",
        "title": "Seasonal Cycle of Idealized Polar Clouds: Large Eddy Simulations Driven by a GCM",
        "author": [
            {
                "family_name": "Zhang",
                "given_name": "Xiyue",
                "orcid": "0000-0002-6031-7830",
                "clpid": "Zhang-Xiyue"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Shen",
                "given_name": "Zhaoyi",
                "orcid": "0000-0002-0444-4720",
                "clpid": "Shen-Zhaoyi"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-Kyle-G"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "orcid": "0000-0003-0190-2869",
                "clpid": "Eisenman-Ian"
            }
        ],
        "abstract": "The uncertainty in polar cloud feedbacks calls for process understanding of the cloud response to climate warming. As an initial step toward improved process understanding, we investigate the seasonal cycle of polar clouds in the current climate by adopting a novel modeling framework using large eddy simulations (LES), which explicitly resolve cloud dynamics. Resolved horizontal and vertical advection of heat and moisture from an idealized general circulation model (GCM) are prescribed as forcing in the LES. The LES are also forced with prescribed sea ice thickness, but surface temperature, atmospheric temperature, and moisture evolve freely without nudging. A semigray radiative transfer scheme without water vapor and cloud feedbacks allows the GCM and LES to achieve closed energy budgets more easily than would be possible with more complex schemes. This enables the mean states in the two models to be consistently compared, without the added complications from interaction with more comprehensive radiation. We show that the LES closely follow the GCM seasonal cycle, and the seasonal cycle of low-level clouds in the LES resembles observations: maximum cloud liquid occurs in late summer and early autumn, and winter clouds are dominated by ice in the upper troposphere. Large-scale advection of moisture provides the main source of water vapor for the liquid-containing clouds in summer, while a temperature advection peak in winter makes the atmosphere relatively dry and reduces cloud condensate. The framework we develop and employ can be used broadly for studying cloud processes and the response of polar clouds to climate warming.",
        "doi": "10.1029/2021MS002671",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modelling Earth Systems",
        "publication_date": "2022-01",
        "series_number": "1",
        "volume": "14",
        "issue": "1",
        "pages": "Art. No. e2021MS002671"
    },
    {
        "id": "authors:jpqx4-32a63",
        "collection": "authors",
        "collection_id": "jpqx4-32a63",
        "cite_using_url": "https://authors.library.caltech.edu/records/jpqx4-32a63",
        "type": "article",
        "title": "Top-of-Atmosphere Albedo Bias from Neglecting Three-Dimensional Cloud Radiative Effects",
        "author": [
            {
                "family_name": "Singer",
                "given_name": "Clare E.",
                "orcid": "0000-0002-1708-0997",
                "clpid": "Singer-Clare-E"
            },
            {
                "family_name": "Lopez-Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895",
                "clpid": "Lopez-Gomez-Ignacio"
            },
            {
                "family_name": "Zhang",
                "given_name": "Xiyue",
                "orcid": "0000-0002-6031-7830",
                "clpid": "Zhang-Xiyue"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "<div>\n<div>\n<div>\n\n\n<p>Clouds cover on average nearly 70% of Earth&rsquo;s surface and regulate the global albedo. The magnitude of the shortwave reflection by clouds depends on their location, optical properties, and three-dimensional (3D) structure. Due to computational limitations, Earth system models are unable to perform 3D radiative transfer calculations. Instead they make assumptions, including the independent column approximation (ICA), that neglect effects of 3D cloud morphology on albedo. We show how the resulting radiative flux bias (ICA-3D) depends on cloud morphology and solar zenith angle. We use high-resolution (20&ndash;100-m horizontal resolution) large-eddy simulations to produce realistic 3D cloud fields covering three dominant regimes of low-latitude clouds: shallow cumulus, marine stratocumulus, and deep convective cumulonimbus. A Monte Carlo code is used to run 3D and ICA broadband radiative transfer calculations; we calculate the top-of-atmosphere (TOA) reflected flux and surface irradiance biases as functions of solar zenith angle for these three cloud regimes. Finally, we use satellite observations of cloud water path (CWP) climatology, and the robust correlation between CWP and TOA flux bias in our LES sample, to roughly estimate the impact of neglecting 3D cloud radiative effects on a global scale. We find that the flux bias is largest at small zenith angles and for deeper clouds, while the albedo bias is most prominent for large zenith angles. In the tropics, the annual-mean shortwave radiative flux bias is estimated to be 3.1 &plusmn; 1.6 W m<sup>&minus;2</sup>, reaching as much as 6.5 W m<sup>&minus;2</sup> locally.</p>\n\n</div>\n</div>\n</div>",
        "doi": "10.1175/JAS-D-21-0032.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2021-12",
        "series_number": "12",
        "volume": "78",
        "issue": "12",
        "pages": "4053-4069"
    },
    {
        "id": "authors:4rsew-ysf10",
        "collection": "authors",
        "collection_id": "4rsew-ysf10",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210518-081155344",
        "type": "article",
        "title": "Constraining the Date of a Seasonally Ice-Free Arctic Using a Simple Model",
        "author": [
            {
                "family_name": "Bonan",
                "given_name": "David B.",
                "orcid": "0000-0003-3867-6009",
                "clpid": "Bonan-David-B"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "orcid": "0000-0003-0190-2869",
                "clpid": "Eisenman-Ian"
            },
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-Robert-C-J"
            }
        ],
        "abstract": "State-of-the-art climate models simulate a large spread in the projected decline of Arctic sea-ice area (SIA) over the 21st century. Here we diagnose causes of this intermodel spread using a simple model that approximates future SIA based on present SIA and the sensitivity of SIA to Arctic temperatures. This model accounts for 70%\u201395% of the intermodel variance, with the majority of the spread arising from present-day biases. The remaining spread arises from intermodel differences in Arctic warming, with some contribution from differences in the local sea-ice sensitivity. Using observations to constrain the projections moves the probability of an ice-free Arctic forward by 10\u201335 years when compared to unconstrained projections. Under a high-emissions scenario, an ice-free Arctic will likely (urn:x-wiley:00948276:media:grl62946:grl62946-math-000166% probability) occur between 2036 and 2056 in September and between 2050 and 2068 from July to October. Under a medium-emissions scenario, the \"likely\" date occurs between 2040 and 2062 in September and much later in the 21st century from July to October.",
        "doi": "10.1029/2021GL094309",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2021-09-20",
        "series_number": "18",
        "volume": "48",
        "issue": "18",
        "pages": "Art. No. e2021GL094309"
    },
    {
        "id": "authors:djfe2-hm225",
        "collection": "authors",
        "collection_id": "djfe2-hm225",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210930-172547442",
        "type": "article",
        "title": "Constraining the Date of a Seasonally Ice\u2010Free Arctic Using a Simple Model",
        "author": [
            {
                "family_name": "Bonan",
                "given_name": "David B.",
                "orcid": "0000-0003-3867-6009",
                "clpid": "Bonan-David-B"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "orcid": "0000-0003-0190-2869",
                "clpid": "Eisenman-Ian"
            },
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-Robert-C-J"
            }
        ],
        "abstract": "State-of-the-art climate models simulate a large spread in the projected decline of Arctic sea-ice area (SIA) over the 21st century. Here we diagnose causes of this intermodel spread using a simple model that approximates future SIA based on present SIA and the sensitivity of SIA to Arctic temperatures. This model accounts for 70%\u201395% of the intermodel variance, with the majority of the spread arising from present-day biases. The remaining spread arises from intermodel differences in Arctic warming, with some contribution from differences in the local sea-ice sensitivity. Using observations to constrain the projections moves the probability of an ice-free Arctic forward by 10\u201335 years when compared to unconstrained projections. Under a high-emissions scenario, an ice-free Arctic will likely (urn:x-wiley:00948276:media:grl62946:grl62946-math-000166% probability) occur between 2036 and 2056 in September and between 2050 and 2068 from July to October. Under a medium-emissions scenario, the \"likely\" date occurs between 2040 and 2062 in September and much later in the 21st century from July to October.",
        "doi": "10.1029/2021gl094309",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2021-09-20",
        "series_number": "18",
        "volume": "48",
        "issue": "18",
        "pages": "Art. No. e2021GL094309"
    },
    {
        "id": "authors:5x2v8-6ma54",
        "collection": "authors",
        "collection_id": "5x2v8-6ma54",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210113-143919927",
        "type": "article",
        "title": "Calibration and Uncertainty Quantification of Convective Parameters in an Idealized GCM",
        "author": [
            {
                "family_name": "Dunbar",
                "given_name": "Oliver R. A.",
                "orcid": "0000-0001-7374-0382",
                "clpid": "Dunbar-Oliver-R-A"
            },
            {
                "family_name": "Garbuno-Inigo",
                "given_name": "Alfredo",
                "orcid": "0000-0003-3279-619X",
                "clpid": "Garbuno-Inigo-Alfredo"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew M.",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            }
        ],
        "abstract": "Parameters in climate models are usually calibrated manually, exploiting only small subsets of the available data. This precludes both optimal calibration and quantification of uncertainties. Traditional Bayesian calibration methods that allow uncertainty quantification are too expensive for climate models; they are also not robust in the presence of internal climate variability. For example, Markov chain Monte Carlo (MCMC) methods typically require O(10\u2075) model runs and are sensitive to internal variability noise, rendering them infeasible for climate models. Here we demonstrate an approach to model calibration and uncertainty quantification that requires only O(10\u00b2) model runs and can accommodate internal climate variability. The approach consists of three stages: (a) a calibration stage uses variants of ensemble Kalman inversion to calibrate a model by minimizing mismatches between model and data statistics; (b) an emulation stage emulates the parameter-to-data map with Gaussian processes (GP), using the model runs in the calibration stage for training; (c) a sampling stage approximates the Bayesian posterior distributions by sampling the GP emulator with MCMC. We demonstrate the feasibility and computational efficiency of this calibrate-emulate-sample (CES) approach in a perfect-model setting. Using an idealized general circulation model, we estimate parameters in a simple convection scheme from synthetic data generated with the model. The CES approach generates probability distributions of the parameters that are good approximations of the Bayesian posteriors, at a fraction of the computational cost usually required to obtain them. Sampling from this approximate posterior allows the generation of climate predictions with quantified parametric uncertainties.",
        "doi": "10.1029/2020MS002454",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modelling Earth Systems",
        "publication_date": "2021-09",
        "series_number": "9",
        "volume": "13",
        "issue": "9",
        "pages": "Art. No. e2020MS002454"
    },
    {
        "id": "authors:kz9pp-mt041",
        "collection": "authors",
        "collection_id": "kz9pp-mt041",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210630-202305416",
        "type": "article",
        "title": "Assessing Biases and Climate Implications of the Diurnal Precipitation Cycle in Climate Models",
        "author": [
            {
                "family_name": "Christopoulos",
                "given_name": "Costa",
                "orcid": "0000-0002-8552-465X",
                "clpid": "Christopoulos-Costa"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The diurnal cycle is a common benchmark for evaluating the performance of weather and climate models on short timescales. For decades, capturing the timing of peak precipitation during the day has remained a challenge for climate models. In this study, the phase and amplitude of the diurnal precipitation cycle in Coupled Model Intercomparison Project (CMIP) models are compared to satellite data. While some improvements align CMIP6 models closer to satellite observations, significant biases in the timing of peak precipitation remain, especially over land. Notably, precipitation over land in CMIP6 models still occurs \u223c5.4 h too early; the diurnal cycle amplitude is \u223c0.81 mm day\u207b\u00b9 too small over the oceans. Further, the diurnal phase of oceanic precipitation correlates weakly with the equilibrium climate sensitivity in CMIP6 models: models with a later precipitation peak over oceans tend to exhibit a higher climate sensitivity. However, it is unclear whether this relationship is robust.",
        "doi": "10.1029/2021gl093017",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2021-07-16",
        "series_number": "13",
        "volume": "48",
        "issue": "13",
        "pages": "Art. No. e2021GL093017"
    },
    {
        "id": "authors:p9gdj-nbk35",
        "collection": "authors",
        "collection_id": "p9gdj-nbk35",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210626-183439679",
        "type": "article",
        "title": "Accelerating progress in climate science",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Jeevanjee",
                "given_name": "Nadir",
                "orcid": "0000-0002-6657-896X",
                "clpid": "Jeevanjee-Nadair"
            },
            {
                "family_name": "Socolow",
                "given_name": "Robert",
                "clpid": "Socolow-Robert"
            }
        ],
        "abstract": "Interdisciplinary teams that integrate theory, data, and computing can now produce urgently needed, action-oriented climate science.",
        "doi": "10.1063/pt.3.4772",
        "issn": "0031-9228",
        "publisher": "American Institute of Physics",
        "publication": "Physics Today",
        "publication_date": "2021-06",
        "series_number": "6",
        "volume": "74",
        "issue": "6",
        "pages": "44-51"
    },
    {
        "id": "authors:1ddr2-aqh54",
        "collection": "authors",
        "collection_id": "1ddr2-aqh54",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210423-164905420",
        "type": "article",
        "title": "Concerning the aims and scope for JAMES",
        "author": [
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "orcid": "0000-0002-3711-236X",
                "clpid": "Griffies-Stephen-M"
            },
            {
                "family_name": "Blyth",
                "given_name": "Eleanor",
                "clpid": "Blyth-Eleanor"
            },
            {
                "family_name": "Fan",
                "given_name": "Jiwen",
                "orcid": "0000-0001-5280-4391",
                "clpid": "Fan-Jiwen"
            },
            {
                "family_name": "Pincus",
                "given_name": "Robert",
                "orcid": "0000-0002-0016-3470",
                "clpid": "Pincus-Robert"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "In this editorial, we present general principles as well as specific notions that guide the strategy of JAMES\u2032 editors in realizing the journal's mission.",
        "doi": "10.1029/2021ms002567",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2021-05",
        "series_number": "5",
        "volume": "13",
        "issue": "5",
        "pages": "Art. No. e2021MS002567"
    },
    {
        "id": "authors:b8w16-kkj37",
        "collection": "authors",
        "collection_id": "b8w16-kkj37",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210503-083240124",
        "type": "article",
        "title": "Predicting the Interannual Variability of California's Total Annual Precipitation",
        "author": [
            {
                "family_name": "Cheng",
                "given_name": "Rui",
                "orcid": "0000-0002-3003-8339",
                "clpid": "Cheng-Rui"
            },
            {
                "family_name": "Novak",
                "given_name": "Lenka",
                "clpid": "Novak-Lenka"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Understanding and predicting precipitation characteristics on seasonal and longer timescales can help California prepare for long\u2010term droughts and precipitation extremes. We find that interannual variations in total precipitation across California are primarily determined by precipitation frequency. As was shown previously for total precipitation, the precipitation frequency is linked to the North Pacific jet stream location. This indicates that California precipitation frequency is primarily controlled by where the jet guides precipitate weather systems rather than how moist or energetic the systems are. The jet's position, in turn, depends on the states of the El Ni\u00f1o\u2010Southern Oscillation (ENSO) and of the Pacific Decadal Oscillation (PDO). We use this to construct a regression model that predicts variations in California's annual total precipitation and precipitation frequency. Up to 20% of the wintertime precipitation variance in Southern California is predictable using decorrelated ENSO and PDO indices in the previous summer.",
        "doi": "10.1029/2020GL091465",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2021-04-16",
        "series_number": "7",
        "volume": "48",
        "issue": "7",
        "pages": "Art. No. e2020GL091465"
    },
    {
        "id": "authors:bym2r-wy864",
        "collection": "authors",
        "collection_id": "bym2r-wy864",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20210611-122858735",
        "type": "article",
        "title": "Is the Surface Salinity Difference between the Atlantic and Indo-Pacific a Signature of the Atlantic Meridional Overturning Circulation?",
        "author": [
            {
                "family_name": "Nilsson",
                "given_name": "Johan",
                "clpid": "Nilsson-Johan"
            },
            {
                "family_name": "Ferreira",
                "given_name": "David",
                "orcid": "0000-0003-3243-9774",
                "clpid": "Ferreira-David"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-Robert-C-J"
            }
        ],
        "abstract": "The high Atlantic surface salinity has sometimes been interpreted as a signature of the Atlantic meridional overturning circulation and an associated salt advection feedback. Here, the role of oceanic and atmospheric processes for creating the surface salinity difference between the Atlantic and Indo-Pacific is examined using observations and a conceptual model. In each basin, zonally averaged data are represented in diagrams relating net evaporation \u02dcE and surface salinity S. The data-pair curves in the \u02dcE\u2013S plane share common features in both basins. However, the slopes of the curves are generally smaller in the Atlantic than in the Indo-Pacific, indicating a weaker sensitivity of the Atlantic surface salinity to net evaporation variations. To interpret these observations, a conceptual advective\u2013diffusive model of the upper-ocean salinity is constructed. Notably, the \u02dcE\u2013S relations can be qualitatively reproduced with only meridional diffusive salt transport. In this limit, the interbasin difference in salinity is caused by the spatial structure of net evaporation, which in the Indo-Pacific oceans contains lower meridional wavenumbers that are weakly damped by the diffusive transport. The observed Atlantic \u02dcE\u2013Srelationship at the surface reveals no clear influence of northward advection associated with the meridional overturning circulation; however, a signature of northward advection emerges in the relationship when the salinity is vertically averaged over the upper kilometer. The results indicate that the zonal-mean near-surface salinity is shaped primarily by the spatial pattern of net evaporation and the diffusive meridional salt transport due to wind-driven gyres and mesoscale ocean eddies, rather than by salt advection within the meridional overturning circulation.",
        "doi": "10.1175/jpo-d-20-0126.1",
        "issn": "0022-3670",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Physical Oceanography",
        "publication_date": "2021-03",
        "series_number": "3",
        "volume": "51",
        "issue": "3",
        "pages": "769-787"
    },
    {
        "id": "authors:grfyb-v6b07",
        "collection": "authors",
        "collection_id": "grfyb-v6b07",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200402-140348174",
        "type": "article",
        "title": "Calibrate, emulate, sample",
        "author": [
            {
                "family_name": "Cleary",
                "given_name": "Emmet",
                "clpid": "Cleary-Emmet"
            },
            {
                "family_name": "Garbuno-Inigo",
                "given_name": "Alfredo",
                "orcid": "0000-0003-3279-619X",
                "clpid": "Garbuno-Inigo-Alfredo"
            },
            {
                "family_name": "Lan",
                "given_name": "Shiwei",
                "orcid": "0000-0002-9167-3715",
                "clpid": "Lan-Shiwei"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew M.",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            }
        ],
        "abstract": "Many parameter estimation problems arising in applications can be cast in the framework of Bayesian inversion. This allows not only for an estimate of the parameters, but also for the quantification of uncertainties in the estimates. Often in such problems the parameter-to-data map is very expensive to evaluate, and computing derivatives of the map, or derivative-adjoints, may not be feasible. Additionally, in many applications only noisy evaluations of the map may be available. We propose an approach to Bayesian inversion in such settings that builds on the derivative-free optimization capabilities of ensemble Kalman inversion methods. The overarching approach is to first use ensemble Kalman sampling (EKS) to calibrate the unknown parameters to fit the data; second, to use the output of the EKS to emulate the parameter-to-data map; third, to sample from an approximate Bayesian posterior distribution in which the parameter-to-data map is replaced by its emulator. This results in a principled approach to approximate Bayesian inference that requires only a small number of evaluations of the (possibly noisy approximation of the) parameter-to-data map. It does not require derivatives of this map, but instead leverages the documented power of ensemble Kalman methods. Furthermore, the EKS has the desirable property that it evolves the parameter ensemble towards the regions in which the bulk of the parameter posterior mass is located, thereby locating them well for the emulation phase of the methodology. In essence, the EKS methodology provides a cheap solution to the design problem of where to place points in parameter space to efficiently train an emulator of the parameter-to-data map for the purposes of Bayesian inversion.",
        "doi": "10.1016/j.jcp.2020.109716",
        "issn": "0021-9991",
        "publisher": "Elsevier",
        "publication": "Journal of Computational Physics",
        "publication_date": "2021-01-01",
        "volume": "424",
        "pages": "Art. No. 109716"
    },
    {
        "id": "authors:d2cbz-tmr38",
        "collection": "authors",
        "collection_id": "d2cbz-tmr38",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20201117-081328944",
        "type": "article",
        "title": "Solar geoengineering may not prevent strong warming from direct effects of CO\u2082 on stratocumulus cloud cover",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-Colleen-M"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-Kyle-G"
            }
        ],
        "abstract": "Discussions of countering global warming with solar geoengineering assume that warming owing to rising greenhouse-gas concentrations can be compensated by artificially reducing the amount of sunlight Earth absorbs. However, solar geoengineering may not be fail-safe to prevent global warming because CO\u2082 can directly affect cloud cover: It reduces cloud cover by modulating the longwave radiative cooling within the atmosphere. This effect is not mitigated by solar geoengineering. Here, we use idealized high-resolution simulations of clouds to show that, even under a sustained solar geoengineering scenario with initially only modest warming, subtropical stratocumulus clouds gradually thin and may eventually break up into scattered cumulus clouds, at concentrations exceeding 1,700 parts per million (ppm). Because stratocumulus clouds cover large swaths of subtropical oceans and cool Earth by reflecting incident sunlight, their loss would trigger strong (about 5 K) global warming. Thus, the results highlight that, at least in this extreme and idealized scenario, solar geoengineering may not suffice to counter greenhouse-gas-driven global warming.",
        "doi": "10.1073/pnas.2003730117",
        "pmcid": "PMC7720182",
        "issn": "0027-8424",
        "publisher": "National Academy of Sciences",
        "publication": "Proceedings of the National Academy of Sciences of the United States of America",
        "publication_date": "2020-12-01",
        "series_number": "48",
        "volume": "117",
        "issue": "48",
        "pages": "30179-30185"
    },
    {
        "id": "authors:x2w3a-2k430",
        "collection": "authors",
        "collection_id": "x2w3a-2k430",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20201015-152734310",
        "type": "article",
        "title": "A Generalized Mixing Length Closure for Eddy-Diffusivity Mass-Flux Schemes of Turbulence and Convection",
        "author": [
            {
                "family_name": "Lopez\u2010Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895",
                "clpid": "Lopez\u2010Gomez-I"
            },
            {
                "family_name": "Cohen",
                "given_name": "Yair",
                "orcid": "0000-0002-9615-2476",
                "clpid": "Cohen-Y"
            },
            {
                "family_name": "He",
                "given_name": "Jia",
                "clpid": "He-Jia"
            },
            {
                "family_name": "Jaruga",
                "given_name": "Anna",
                "orcid": "0000-0003-3194-6440",
                "clpid": "Jaruga-Anna"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Because of their limited spatial resolution, numerical weather prediction and climate models have to rely on parameterizations to represent atmospheric turbulence and convection. Historically, largely independent approaches have been used to represent boundary layer turbulence and convection, neglecting important interactions at the subgrid scale. Here we build on an eddy\u2010diffusivity mass\u2010flux (EDMF) scheme that represents all subgrid\u2010scale mixing in a unified manner, partitioning subgrid\u2010scale fluctuations into contributions from local diffusive mixing and coherent advective structures and allowing them to interact within a single framework. The EDMF scheme requires closures for the interaction between the turbulent environment and the plumes and for local mixing. A second\u2010order equation for turbulence kinetic energy (TKE) provides one ingredient for the diffusive local mixing closure, leaving a mixing length to be parameterized. Here, we propose a new mixing length formulation, based on constraints derived from the TKE balance. It expresses local mixing in terms of the same physical processes in all regimes of boundary layer flow. The formulation is tested at a range of resolutions and across a wide range of boundary layer regimes, including a stably stratified boundary layer, a stratocumulus\u2010topped marine boundary layer, and dry convection. Comparison with large eddy simulations (LES) shows that the EDMF scheme with this diffusive mixing parameterization accurately captures the structure of the boundary layer and clouds in all cases considered.",
        "doi": "10.1029/2020ms002161",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2020-11",
        "series_number": "11",
        "volume": "12",
        "issue": "11",
        "pages": "Art. No. e2020MS002161"
    },
    {
        "id": "authors:mqh7j-b8e38",
        "collection": "authors",
        "collection_id": "mqh7j-b8e38",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200729-145256584",
        "type": "article",
        "title": "Pattern Recognition Methods to Separate Forced Responses from Internal Variability in Climate Model Ensembles and Observations",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "clpid": "Wills-R-C-J"
            },
            {
                "family_name": "Battisti",
                "given_name": "David S.",
                "orcid": "0000-0003-4871-1293",
                "clpid": "Battisti-D-S"
            },
            {
                "family_name": "Armour",
                "given_name": "Kyle C.",
                "orcid": "0000-0002-6833-5179",
                "clpid": "Armour-K-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Deser",
                "given_name": "Clara",
                "orcid": "0000-0002-5517-9103",
                "clpid": "Deser-C"
            }
        ],
        "abstract": "Ensembles of climate model simulations are commonly used to separate externally forced climate change from internal variability. However, much of the information gained from running large ensembles is lost in traditional methods of data reduction such as linear trend analysis or large-scale spatial averaging. This paper demonstrates how a pattern recognition method (signal-to-noise-maximizing pattern filtering) extracts patterns of externally forced climate change from large ensembles and identifies the forced climate response with up to ten times fewer ensemble members than simple ensemble averaging. It is particularly effective at filtering out spatially coherent modes of internal variability (e.g., El Ni\u00f1o, North Atlantic Oscillation), which would otherwise alias into estimates of regional responses to forcing. This method is used to identify forced climate responses within the 40-member Community Earth System Model (CESM) large ensemble, including an El-Ni\u00f1o-like response to volcanic eruptions and forced trends in the North Atlantic Oscillation. The ensemble-based estimate of the forced response is used to test statistical methods for isolating the forced response from a single realization (i.e., individual ensemble members). Low-frequency pattern filtering is found to skillfully identify the forced response within individual ensemble members and is applied to the HadCRUT4 reconstruction of observed temperatures, whereby it identifies slow components of observed temperature changes that are consistent with the expected effects of anthropogenic greenhouse gas and aerosol forcing.",
        "doi": "10.1175/JCLI-D-19-0855.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2020-10-15",
        "series_number": "20",
        "volume": "33",
        "issue": "20",
        "pages": "8693-8719"
    },
    {
        "id": "authors:5dasa-44z38",
        "collection": "authors",
        "collection_id": "5dasa-44z38",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200610-102248992",
        "type": "article",
        "title": "Sensitivity of idealized mixed-phase stratocumulus to climate perturbations",
        "author": [
            {
                "family_name": "Zhang",
                "given_name": "Xiyue",
                "orcid": "0000-0002-6031-7830",
                "clpid": "Zhang-Xiyue"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-Colleen-M"
            }
        ],
        "abstract": "Large eddy simulations (LES) that explicitly resolve boundary layer (BL) turbulence and clouds are used to explore the sensitivity of idealized Arctic BL clouds to climate perturbations. The LES focus on conditions resembling springtime, when surface heat fluxes over sea ice are weak, and the cloud radiative effect is dominated by the longwave effect. In the LES, the condensed water path increases with BL temperature and free\u2010tropospheric relative humidity, but it decreases with inversion strength. The dependencies of cloud properties on environmental variables exhibited by the LES can largely be reproduced by a mixed\u2010layer model. Mixed\u2010layer model analysis shows that the liquid water path increases with warming because the liquid water gradient increase under warming overcompensates for geometric cloud thinning. This response contrasts with the response of subtropical stratocumulus to warming, whose liquid water path decreases as the clouds thin geometrically under warming. The results suggest that methods used to explain the response of lower\u2010latitude BL clouds to climate change can also elucidate changes in idealized Arctic BL clouds, although subtropical and Arctic clouds occupy different thermodynamic regimes.",
        "doi": "10.1002/qj.3846",
        "issn": "0035-9009",
        "publisher": "Wiley",
        "publication": "Quarterly Journal of the Royal Meteorological Society",
        "publication_date": "2020-10",
        "series_number": "732",
        "volume": "146",
        "issue": "732",
        "pages": "3285-3305"
    },
    {
        "id": "authors:fy6f4-9fb09",
        "collection": "authors",
        "collection_id": "fy6f4-9fb09",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200820-123726127",
        "type": "article",
        "title": "Unified Entrainment and Detrainment Closures for Extended Eddy-Diffusivity Mass-Flux Schemes",
        "author": [
            {
                "family_name": "Cohen",
                "given_name": "Yair",
                "orcid": "0000-0002-9615-2476",
                "clpid": "Cohen-Yair"
            },
            {
                "family_name": "Lopez\u2010Gomez",
                "given_name": "Ignacio",
                "orcid": "0000-0002-7255-5895",
                "clpid": "Lopez\u2010Gomez-Ignacio"
            },
            {
                "family_name": "Jaruga",
                "given_name": "Anna",
                "orcid": "0000-0003-3194-6440",
                "clpid": "Jaruga-Anna"
            },
            {
                "family_name": "He",
                "given_name": "Jia",
                "clpid": "He-Jia"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-Colleen-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "We demonstrate that an extended eddy\u2010diffusivity mass\u2010flux (EDMF) scheme can be used as a unified parameterization of subgrid\u2010scale turbulence and convection across a range of dynamical regimes, from dry convective boundary layers, through shallow convection, to deep convection. Central to achieving this unified representation of subgrid\u2010scale motions are entrainment and detrainment closures. We model entrainment and detrainment rates as a combination of turbulent and dynamical processes. Turbulent entrainment/detrainment is represented as downgradient diffusion between plumes and their environment. Dynamical entrainment/detrainment is proportional to a ratio of a relative buoyancy of a plume and a vertical velocity scale, that is modulated by heuristic nondimensional functions which represent their relative magnitudes and the enhanced detrainment due to evaporation from clouds in drier environment. We first evaluate the closures off\u2010line against entrainment and detrainment rates diagnosed from large eddy simulations (LESs) in which tracers are used to identify plumes, their turbulent environment, and mass and tracer exchanges between them. The LES are of canonical test cases of a dry convective boundary layer, shallow convection, and deep convection, thus spanning a broad rangeof regimes. We then compare the LES with the full EDMF scheme, including the new closures, in a single\u2010column model (SCM). The results show good agreement between the SCM and LES in quantities that are key for climate models, including thermodynamic profiles, cloud liquid water profiles, and profiles of higher moments of turbulent statistics. The SCM also captures well the diurnal cycle of convection and the onset of precipitation.",
        "doi": "10.1029/2020ms002162",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2020-09",
        "series_number": "9",
        "volume": "12",
        "issue": "9",
        "pages": "Art. No. e2020MS002162"
    },
    {
        "id": "authors:vy253-exf87",
        "collection": "authors",
        "collection_id": "vy253-exf87",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200819-095025315",
        "type": "article",
        "title": "A Continuous Record of Central Tropical Pacific Climate Since the Midnineteenth Century Reconstructed From Fanning and Palmyra Island Corals: A Case Study in Coral Data Reanalysis",
        "author": [
            {
                "family_name": "Sanchez",
                "given_name": "S. C.",
                "orcid": "0000-0002-1923-1218",
                "clpid": "Sanchez-Sara-C"
            },
            {
                "family_name": "Westphal",
                "given_name": "N.",
                "orcid": "0000-0001-6343-5755",
                "clpid": "Westphal-Niko"
            },
            {
                "family_name": "Haug",
                "given_name": "G. H.",
                "clpid": "Haug-Gerald-H"
            },
            {
                "family_name": "Cheng",
                "given_name": "H.",
                "clpid": "Cheng-H"
            },
            {
                "family_name": "Edwards",
                "given_name": "R. L.",
                "clpid": "Edwards-R-Lawrence"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Cobb",
                "given_name": "K. M.",
                "orcid": "0000-0002-2125-9164",
                "clpid": "Cobb-Kim-M"
            },
            {
                "family_name": "Charles",
                "given_name": "C. D.",
                "orcid": "0000-0003-4016-2365",
                "clpid": "Charles-Christopher-D"
            }
        ],
        "abstract": "Accurate estimation of central tropical Pacific (CTP) climate variability on interannual to centennial time scales is required for robust projections of future global climate trends. Here we outline an approach that blends instrumental and coral proxy observations to yield a continuous, monthly resolved record of climate evolution in the CTP spanning the past 160 years. We concatenate coral oxygen isotope (\u03b4\u00b9\u2078O) records from multiple living and fossil corals collected from Fanning Island (4\u00b0N, 160\u00b0W) and Palmyra Island (5\u00b0N; 162\u00b0W) located in the heart of the El Ni\u00f1o\u2013Southern Oscillation. We use the regularized expectation maximization (RegEM) method to impute missing data across short gaps of 5 to 23 years within and beyond individual coral records. The resulting monthly resolved Fanning/Palmyra Island climate record spans continuously from 1863 to 2016 and provides an example of how extended time series can be built from shorter coral segments. The extended record highlights the strong trend toward warmer and wetter mean conditions in late twentieth century, in agreement with the majority of climate model hindcast simulations. The continuous reconstruction also enables a direct comparison of four exceptionally strong El Ni\u00f1o events (1877\u20131878, 1940\u20131941, 1997\u20131998, and 2015\u20132016). Three of these very strong El Ni\u00f1o events in the CTP featured a precursor warm event in the prior year and that may have favored the development of a strong El Ni\u00f1o event.",
        "doi": "10.1029/2020pa003848",
        "issn": "2572-4517",
        "publisher": "American Geophysical Union",
        "publication": "Paleoceanography and Paleoclimatology",
        "publication_date": "2020-08",
        "series_number": "8",
        "volume": "35",
        "issue": "8",
        "pages": "Art. No. e2020PA003848"
    },
    {
        "id": "authors:86hqv-p1261",
        "collection": "authors",
        "collection_id": "86hqv-p1261",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200220-100007967",
        "type": "article",
        "title": "Atmospheric Circulation Response to Short-Term Arctic Warming in an Idealized Model",
        "author": [
            {
                "family_name": "Hell",
                "given_name": "Momme C.",
                "clpid": "Hell-M-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Li",
                "given_name": "Camille",
                "clpid": "Li-Camille"
            }
        ],
        "abstract": "Recent Arctic sea ice loss in fall has been posited to drive midlatitude circulation changes into winter and even spring. Past work has shown that sea ice loss can indeed trigger a weakening of the stratospheric polar vortex, which can lead to delayed surface weather changes. But the mechanisms of such changes and their relevant time scales have remained unclear. This study uses large ensembles of idealized GCM simulations to identify how and over what time scales the atmospheric circulation responds to short-term surface heat flux changes in high latitudes. The ensemble-mean response of the atmospheric circulation is approximately linear in the amplitude of the surface forcing. It is also insensitive to whether the forcing is zonally asymmetric or symmetric, that is, whether stationary waves are generated or not. The circulation response can be decomposed into a rapid thermal response and a slower dynamic adjustment. The adjustment arises through weakening of vertical wave activity fluxes from the troposphere into the stratosphere in response to polar warming, a mechanism that differs from sudden stratospheric warmings yet still results in a weakened stratospheric circulation. The stratospheric response is delayed and persists for about 2 months because the thermal response of the stratosphere is slow compared with that of the troposphere. The delayed stratospheric response feeds back onto the troposphere, but the tropospheric effects are weak compared with natural variability. The general pathway for the delayed response appears to be relatively independent of the atmospheric background state at the time of the anomalous surface forcing.",
        "doi": "10.1175/jas-d-19-0133.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2020-02",
        "series_number": "2",
        "volume": "77",
        "issue": "2",
        "pages": "531-549"
    },
    {
        "id": "authors:84b8v-j3z86",
        "collection": "authors",
        "collection_id": "84b8v-j3z86",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200127-131857757",
        "type": "article",
        "title": "Statistically Steady State Large\u2010Eddy Simulations Forced by an Idealized GCM: 1. Forcing Framework and Simulation Characteristics",
        "author": [
            {
                "family_name": "Shen",
                "given_name": "Zhaoyi",
                "orcid": "0000-0002-0444-4720",
                "clpid": "Shen-Zhaoyi"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            },
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Using large\u2010eddy simulations (LES) systematically has the potential to inform parameterizations of subgrid\u2010scale processes in general circulation models (GCMs), such as turbulence, convection, and clouds. Here we show how LES can be run to simulate grid columns of GCMs to generate LES across a cross section of dynamical regimes. The LES setup approximately replicates the thermodynamic and water budgets in GCM grid columns. Resolved horizontal and vertical transports of heat and water and large\u2010scale pressure gradients from the GCM are prescribed as forcing in the LES. The LES are forced with prescribed surface temperatures, but atmospheric temperature and moisture are free to adjust, reducing the imprinting of GCM fields on the LES. In both the GCM and LES, radiative transfer is treated in a unified but idealized manner (semigray atmosphere without water vapor feedback or cloud radiative effects). We show that the LES in this setup reaches statistically steady states without nudging to thermodynamic GCM profiles. The steady states provide training data for developing GCM parameterizations. The same LES setup also provides a good basis for studying the cloud response to global warming.",
        "doi": "10.1029/2019MS001814",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2020-02",
        "series_number": "2",
        "volume": "12",
        "issue": "2",
        "pages": "Art. No. e2019MS001814"
    },
    {
        "id": "authors:sm8p5-7g948",
        "collection": "authors",
        "collection_id": "sm8p5-7g948",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20200109-083234021",
        "type": "article",
        "title": "Midwinter Suppression of Storm Tracks in an Idealized Zonally Symmetric Setting",
        "author": [
            {
                "family_name": "Novak",
                "given_name": "Lenka",
                "clpid": "Novak-L"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Ait-Chaalal",
                "given_name": "Farid",
                "clpid": "Ait-Chaalal-F"
            }
        ],
        "abstract": "The midwinter suppression of eddy activity in the North Pacific storm track is a phenomenon that has resisted reproduction in idealized models that are initialized independently of the observed atmosphere. Attempts at explaining it have often focused on local mechanisms that depend on zonal asymmetries, such as effects of topography on the mean flow and eddies. Here an idealized aquaplanet GCM is used to demonstrate that a midwinter suppression can also occur in the activity of a statistically zonally symmetric storm track. For a midwinter suppression to occur, it is necessary that parameters, such as the thermal inertia of the upper ocean and the strength of tropical ocean energy transport, are chosen suitably to produce a pronounced seasonal cycle of the subtropical jet characteristics. If the subtropical jet is sufficiently strong and located close to the midlatitude storm track during midwinter, it dominates the upper-level flow and guides eddies equatorward, away from the low-level area of eddy generation. This inhibits the baroclinic interaction between upper and lower levels within the storm track and weakens eddy activity. However, as the subtropical jet continues to move poleward during late winter in the idealized GCM (and unlike what is observed), eddy activity picks up again, showing that the properties of the subtropical jet that give rise to the midwinter suppression are subtle. The idealized GCM simulations provide a framework within which possible mechanisms giving rise to a midwinter suppression of storm tracks can be investigated systematically.",
        "doi": "10.1175/JAS-D-18-0353.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2020-01",
        "series_number": "1",
        "volume": "77",
        "issue": "1",
        "pages": "297-313"
    },
    {
        "id": "authors:sdght-7dh46",
        "collection": "authors",
        "collection_id": "sdght-7dh46",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190709-091307243",
        "type": "article",
        "title": "Both differential and equatorial heating contributed to African monsoon variations during the mid-Holocene",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Enzel",
                "given_name": "Yehouda",
                "orcid": "0000-0001-8367-9255",
                "clpid": "Enzel-Y"
            },
            {
                "family_name": "Quade",
                "given_name": "Jay",
                "clpid": "Quade-J"
            }
        ],
        "abstract": "The Sahara was significantly greener 11-5 kya and during multiple earlier interglacial periods. But the mechanisms related to the greening of the Sahara remain uncertain as most climate models severely underestimate past wet conditions over north Africa. The variations in the African monsoon related to the greening of the Sahara are thought to be associated with the variations in the inter-hemispheric differential heating of Earth, caused by orbital variations. However, how orbital variations affect regional climate is not well understood. Using recent theory that relates the position of the tropical rain belt to the atmospheric energy budget, we study the effect of orbital forcing during the mid-Holocene on the African monsoon in simulations provided by the third phase of the Paleo Model Intercomparison Project (PMIP3). We find that energy fluxes in the African sector are related to orbital forcing in a complex manner. Contrary to generally accepted theory, orbital modulation of seasonal differential heating alone is shown to be a weak driver of African monsoon variations. Instead, net atmospheric heating near the equator, which modulates the intensity and extent of seasonal migrations of the tropical rain belt, is an important but overlooked driver of African monsoon variations. A conceptual framework that relates African monsoon variations to both equatorial and inter-hemispheric differential solar heating is presented.",
        "doi": "10.1016/j.epsl.2019.06.019",
        "issn": "0012-821X",
        "publisher": "Elsevier",
        "publication": "Earth and Planetary Science Letters",
        "publication_date": "2019-09-15",
        "volume": "522",
        "pages": "20-29"
    },
    {
        "id": "authors:z0fef-bcz03",
        "collection": "authors",
        "collection_id": "z0fef-bcz03",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20190108-130913145",
        "type": "article",
        "title": "Possible climate transitions from breakup of stratocumulus decks under greenhouse warming",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-C-M"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            }
        ],
        "abstract": "Stratocumulus clouds cover 20% of the low-latitude oceans and are especially prevalent in the subtropics. They cool the Earth by shading large portions of its surface from sunlight. However, as their dynamical scales are too small to be resolvable in global climate models, predictions of their response to greenhouse warming have remained uncertain. Here we report how stratocumulus decks respond to greenhouse warming in large-eddy simulations that explicitly resolve cloud dynamics in a representative subtropical region. In the simulations, stratocumulus decks become unstable and break up into scattered clouds when CO_2 levels rise above 1,200\u2009ppm. In addition to the warming from rising CO_2 levels, this instability triggers a surface warming of about 8\u2009K globally and 10\u2009K in the subtropics. Once the stratocumulus decks have broken up, they only re-form once CO_2 concentrations drop substantially below the level at which the instability first occurred. Climate transitions that arise from this instability may have contributed importantly to hothouse climates and abrupt climate changes in the geological past. Such transitions to a much warmer climate may also occur in the future if CO_2 levels continue to rise.",
        "doi": "10.1038/s41561-019-0310-1",
        "issn": "1752-0894",
        "publisher": "Nature Publishing Group",
        "publication": "Nature Geoscience",
        "publication_date": "2019-03",
        "series_number": "3",
        "volume": "12",
        "issue": "3",
        "pages": "163-167"
    },
    {
        "id": "authors:2z7gz-vc951",
        "collection": "authors",
        "collection_id": "2z7gz-vc951",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180822-092424875",
        "type": "article",
        "title": "Mechanisms Setting the Strength of Orographic Rossby Waves across a Wide Range of Climates in a Moist Idealized GCM",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C. J.",
                "clpid": "Wills-R-C-J"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Orographic stationary Rossby waves are an important influence on the large-scale circulation of the atmosphere, especially in Northern Hemisphere winter. Changes in stationary waves with global warming have the potential to modify patterns of surface temperature and precipitation. This paper presents an analysis of the forcing of stationary waves by midlatitude orography across a wide range of climates in a moist idealized GCM, where latent heating and transient eddies are allowed to feed back on the stationary-eddy dynamics. The stationary-eddy amplitude depends to leading order on the surface winds impinging on the orography, resulting in different climate change responses for mountains at different latitudes. Latent heating is found to damp orographic stationary waves, whereas transient eddies are found to reinforce them. As the climate warms, the damping by latent heating becomes more effective while the reinforcement by transient eddies becomes less effective, leading to an overall reduction in orographic stationary wave amplitude. These effects overwhelm the influences of a reduced meridional temperature gradient and increased dry static stability, both of which increase the sensitivity of the free troposphere to orographic forcing. Together with a reduction in the midlatitude meridional temperature gradient, the weakening of orographic stationary waves leads to reduced zonal asymmetry of temperature and net precipitation in warm, moist climates. While circulation changes in this idealized model cannot be expected to agree quantitatively with changes in the real world, the key physical processes identified are broadly relevant.",
        "doi": "10.1175/JCLI-D-17-0700.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2018-09-15",
        "series_number": "18",
        "volume": "31",
        "issue": "18",
        "pages": "7679-7700"
    },
    {
        "id": "authors:wn8me-3vc56",
        "collection": "authors",
        "collection_id": "wn8me-3vc56",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180711-153419610",
        "type": "article",
        "title": "Eddy Lifetime, Number, and Diffusivity and the Suppression of Eddy Kinetic Energy in Midwinter",
        "author": [
            {
                "family_name": "Schemm",
                "given_name": "Sebatian",
                "clpid": "Schemm-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The wintertime evolution of the North Pacific storm track appears to challenge classical theories of baroclinic instability, which predict deeper extratropical cyclones when baroclinicity is highest. Although the surface baroclinicity peaks during midwinter, and the jet is strongest, eddy kinetic energy (EKE) and baroclinic conversion rates have a midwinter minimum over the North Pacific. This study investigates how the reduction in EKE translates into a reduction in eddy potential vorticity (PV) and heat fluxes via changes in eddy diffusivity. Additionally, it augments previous observations of the midwinter storm-track evolution in both hemispheres using climatologies of tracked surface cyclones. In the North Pacific, the number of surface cyclones is highest during midwinter, while the mean EKE per cyclone and the eddy lifetime are reduced. The midwinter reduction in upper-level eddy activity hence is not associated with a reduction in surface cyclone numbers. North Pacific eddy diffusivities exhibit a midwinter reduction at upper levels, where the Lagrangian decorrelation time is shortest (consistent with reduced eddy lifetimes) and the meridional parcel velocity variance is reduced (consistent with reduced EKE). The resulting midwinter reduction in North Pacific eddy diffusivities translates into an eddy PV flux suppression. In contrast, in the North Atlantic, a milder reduction in the decorrelation time is offset by a maximum in velocity variance, preventing a midwinter diffusivity minimum. The results suggest that a focus on causes of the wintertime evolution of Lagrangian decorrelation times and parcel velocity variance will be fruitful for understanding causes of seasonal storm-track variations.",
        "doi": "10.1175/JCLI-D-17-0644.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2018-07-15",
        "series_number": "14",
        "volume": "31",
        "issue": "14",
        "pages": "5649-5665"
    },
    {
        "id": "authors:ezxta-nxz91",
        "collection": "authors",
        "collection_id": "ezxta-nxz91",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180705-143240657",
        "type": "article",
        "title": "Regional and seasonal variations of the double-ITCZ bias in CMIP5 models",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Brient",
                "given_name": "Florent",
                "clpid": "Brient-Florent"
            }
        ],
        "abstract": "Current climate models represent the zonal- and annual-mean intertropical convergence zone (ITCZ) position in a biased way, with an unrealistic double precipitation peak straddling the equator in the ensemble mean over the models. This bias is seasonally and regionally localized. It results primarily from two regions: the eastern Pacific and Atlantic (EPA), where the ITCZ in boreal winter and spring is displaced farther south than is observed; and the western Pacific (WP), where a more pronounced and wider than observed double ITCZ straddles the equator year-round. Additionally, the precipitation associated with the ascending branches of the zonal overturning circulations (e.g., Walker circulation) in the Pacific and Atlantic sectors is shifted westward. We interpret these biases in light of recent theories that relate the ITCZ position to the atmospheric energy budget. WP biases are associated with the well known Pacific cold tongue bias, which, in turn, is linked to atmospheric net energy input biases near the equator. In contrast, EPA biases are shown to be associated with a positive bias in the cross-equatorial divergent atmospheric energy transport during boreal winter and spring, with two potential sources: tropical biases associated with equatorial sea surface temperatures (SSTs) and tropical low clouds, and extratropical biases associated with Southern Ocean clouds and north Atlantic SST. The distinct seasonal and regional characteristics of WP and EPA biases and the differences in their associated energy budget biases suggest that the biases in the two sectors involve different mechanisms and potentially different sources.",
        "doi": "10.1007/s00382-017-3909-1",
        "issn": "0930-7575",
        "publisher": "Springer",
        "publication": "Climate Dynamics",
        "publication_date": "2018-07",
        "series_number": "1-2",
        "volume": "51",
        "issue": "1-2",
        "pages": "101-117"
    },
    {
        "id": "authors:338r7-ade88",
        "collection": "authors",
        "collection_id": "338r7-ade88",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180316-101647631",
        "type": "article",
        "title": "Atlantic-Pacific Asymmetry in Deep-Water Formation",
        "author": [
            {
                "family_name": "Ferreira",
                "given_name": "David",
                "orcid": "0000-0003-3243-9774",
                "clpid": "Ferreira-D"
            },
            {
                "family_name": "Cessi",
                "given_name": "Paola",
                "clpid": "Cessi-P"
            },
            {
                "family_name": "Coxall",
                "given_name": "Helen K.",
                "clpid": "Coxall-H-K"
            },
            {
                "family_name": "de Boer",
                "given_name": "Agatha",
                "clpid": "de-Boer-A"
            },
            {
                "family_name": "Dijkstra",
                "given_name": "Henk A.",
                "clpid": "Dijkstra-H-A"
            },
            {
                "family_name": "Drijfhout",
                "given_name": "Sybren S.",
                "clpid": "Drijfhout-S-S"
            },
            {
                "family_name": "Eldevik",
                "given_name": "Tor",
                "clpid": "Eldevik-T"
            },
            {
                "family_name": "Harnik",
                "given_name": "Nili",
                "clpid": "Harnik-Nili"
            },
            {
                "family_name": "McManus",
                "given_name": "Jerry F.",
                "orcid": "0000-0002-7365-1600",
                "clpid": "McManus-J-F"
            },
            {
                "family_name": "Marshall",
                "given_name": "David P.",
                "clpid": "Marshall-D-P"
            },
            {
                "family_name": "Nilsson",
                "given_name": "Johan",
                "clpid": "Nilsson-J"
            },
            {
                "family_name": "Roquet",
                "given_name": "Fabien",
                "clpid": "Roquet-F"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            }
        ],
        "abstract": "While the Atlantic Ocean is ventilated by high-latitude deep water formation and exhibits a pole-to-pole overturning circulation, the Pacific Ocean does not. This asymmetric global overturning pattern has persisted for the past 2\u20133 million years, with evidence for different ventilation modes in the deeper past. In the current climate, the Atlantic-Pacific asymmetry occurs because the Atlantic is more saline, enabling deep convection. To what extent the salinity contrast between the two basins is dominated by atmospheric processes (larger net evaporation over the Atlantic) or oceanic processes (salinity transport into the Atlantic) remains an outstanding question. Numerical simulations have provided support for both mechanisms; observations of the present climate support a strong role for atmospheric processes as well as some modulation by oceanic processes. A major avenue for future work is the quantification of the various processes at play to identify which mechanisms are primary in different climate states.",
        "doi": "10.1146/annurev-earth-082517-010045",
        "issn": "0084-6597",
        "publisher": "Annual Reviews",
        "publication": "Annual Review of Earth and Planetary Sciences",
        "publication_date": "2018-05",
        "volume": "46",
        "pages": "327-352"
    },
    {
        "id": "authors:xk6qm-8fe08",
        "collection": "authors",
        "collection_id": "xk6qm-8fe08",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180425-165415428",
        "type": "article",
        "title": "Atmospheric Dynamics Feedback: Concept, Simulations, and Climate Implications",
        "author": [
            {
                "family_name": "Byrne",
                "given_name": "Michael P.",
                "clpid": "Byrne-M-P"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The regional climate response to radiative forcing is largely controlled by changes in the atmospheric circulation. It has been suggested that global climate sensitivity also depends on the circulation response, an effect called the \"atmospheric dynamics feedback.\" Using a technique to isolate the influence of changes in atmospheric circulation on top-of-the-atmosphere radiation, the authors calculate the atmospheric dynamics feedback in coupled climate models. Large-scale circulation changes contribute substantially to all-sky and cloud feedbacks in the tropics but are relatively less important at higher latitudes. Globally averaged, the atmospheric dynamics feedback is positive and amplifies the near-surface temperature response to climate change by an average of 8% in simulations with coupled models. A constraint related to the atmospheric mass budget results in the dynamics feedback being small on large scales relative to feedbacks associated with thermodynamic processes. Idealized-forcing simulations suggest that circulation changes at high latitudes are potentially more effective at influencing global temperature than circulation changes at low latitudes, and the implications for past and future climate change are discussed.",
        "doi": "10.1175/JCLI-D-17-0470.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2018-04-15",
        "series_number": "8",
        "volume": "31",
        "issue": "8",
        "pages": "3249-3264"
    },
    {
        "id": "authors:vhfwf-zka04",
        "collection": "authors",
        "collection_id": "vhfwf-zka04",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180129-142103724",
        "type": "article",
        "title": "Disentangling global warming, multi-decadal variability, and El Ni\u00f1o in Pacific temperatures",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Wallace",
                "given_name": "John M.",
                "clpid": "Wallace-J-M"
            },
            {
                "family_name": "Battisti",
                "given_name": "David S.",
                "orcid": "0000-0003-4871-1293",
                "clpid": "Battisti-D-S"
            },
            {
                "family_name": "Hartmann",
                "given_name": "Dennis L.",
                "orcid": "0000-0002-4495-7774",
                "clpid": "Hartmann-D-L"
            }
        ],
        "abstract": "A key challenge in climate science is to separate observed temperature changes into components due to internal variability and responses to external forcing. Extended integrations of forced and unforced climate models are often used for this purpose. Here we demonstrate a novel method to separate modes of internal variability from global warming based on differences in time scale and spatial pattern, without relying on climate models. We identify uncorrelated components of Pacific sea surface temperature variability due to global warming, the Pacific Decadal Oscillation (PDO), and the El Ni\u00f1o\u2013Southern Oscillation (ENSO). Our results give statistical representations of PDO and ENSO that are consistent with their being separate processes, operating on different time scales, but are otherwise consistent with canonical definitions. We isolate the multidecadal variability of the PDO and find that it is confined to midlatitudes; tropical sea surface temperatures and their teleconnections mix in higher\u2010frequency variability. This implies that midlatitude PDO anomalies are more persistent than previously thought.",
        "doi": "10.1002/2017GL076327",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2018-03-16",
        "series_number": "5",
        "volume": "45",
        "issue": "5",
        "pages": "2487-2496"
    },
    {
        "id": "authors:7z88e-hcv44",
        "collection": "authors",
        "collection_id": "7z88e-hcv44",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180411-105304038",
        "type": "article",
        "title": "Disentangling Global Warming, Multidecadal Variability, and El Ni\u00f1o in Pacific Temperatures",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Wallace",
                "given_name": "John M.",
                "clpid": "Wallace-J-M"
            },
            {
                "family_name": "Battisti",
                "given_name": "David S.",
                "orcid": "0000-0003-4871-1293",
                "clpid": "Battisti-D-S"
            },
            {
                "family_name": "Hartmann",
                "given_name": "Dennis L.",
                "orcid": "0000-0002-4495-7774",
                "clpid": "Hartmann-D-L"
            }
        ],
        "abstract": "A key challenge in climate science is to separate observed temperature changes into components due to internal variability and responses to external forcing. Extended integrations of forced and unforced climate models are often used for this purpose. Here we demonstrate a novel method to separate modes of internal variability from global warming based on differences in time scale and spatial pattern, without relying on climate models. We identify uncorrelated components of Pacific sea surface temperature variability due to global warming, the Pacific Decadal Oscillation (PDO), and the El Ni\u00f1o\u2013Southern Oscillation (ENSO). Our results give statistical representations of PDO and ENSO that are consistent with their being separate processes, operating on different time scales, but are otherwise consistent with canonical definitions. We isolate the multidecadal variability of the PDO and find that it is confined to midlatitudes; tropical sea surface temperatures and their teleconnections mix in higher\u2010frequency variability. This implies that midlatitude PDO anomalies are more persistent than previously thought.",
        "doi": "10.1002/2017GL076327",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2018-03-16",
        "series_number": "5",
        "volume": "45",
        "issue": "5",
        "pages": "2487-2496"
    },
    {
        "id": "authors:t78xa-4n187",
        "collection": "authors",
        "collection_id": "t78xa-4n187",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180206-095908216",
        "type": "article",
        "title": "An Extended Eddy-Diffusivity Mass-Flux Scheme for Unified Representation of Subgrid-Scale Turbulence and Convection",
        "author": [
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-C-M"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            },
            {
                "family_name": "Cohen",
                "given_name": "Yair",
                "orcid": "0000-0002-9615-2476",
                "clpid": "Cohen-Y"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Teixeira",
                "given_name": "Jo\u00e3o",
                "clpid": "Teixeira-J"
            }
        ],
        "abstract": "Large-scale weather forecasting and climate models are beginning to reach horizontal resolutions of kilometers, at which common assumptions made in existing parameterization schemes of subgrid-scale turbulence and convection\u2014such as that they adjust instantaneously to changes in resolved-scale dynamics\u2014cease to be justifiable. Additionally, the common practice of representing boundary-layer turbulence, shallow convection, and deep convection by discontinuously different parameterizations schemes, each with its own set of parameters, has contributed to the proliferation of adjustable parameters in large-scale models. Here we lay the theoretical foundations for an extended eddy-diffusivity mass flux (EDMF) scheme that has explicit time-dependence and memory of subgrid-scale variables and is designed to represent all subgrid-scale turbulence and convection, from boundary layer dynamics to deep convection, in a unified manner. Coherent up- and downdrafts in the scheme are represented as prognostic plumes that interact with their environment and potentially with each other through entrainment and detrainment. The more isotropic turbulence in their environment is represented through diffusive fluxes, with diffusivities obtained from a turbulence kinetic energy budget that consistently partitions turbulence kinetic energy between plumes and environment. The cross-sectional area of up- and downdrafts satisfies a prognostic continuity equation, which allows the plumes to cover variable and arbitrarily large fractions of a large-scale grid box and to have life cycles governed by their own internal dynamics. Relatively simple preliminary proposals for closure parameters are presented and are shown to lead to a successful simulation of shallow convection, including a time-dependent life cycle.",
        "doi": "10.1002/2017MS001162",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2018-03",
        "series_number": "3",
        "volume": "10",
        "issue": "3",
        "pages": "770-800"
    },
    {
        "id": "authors:4k7dz-36k70",
        "collection": "authors",
        "collection_id": "4k7dz-36k70",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20180509-105945938",
        "type": "article",
        "title": "Linking Hadley Circulation and Storm Tracks in a Conceptual Model of the Atmospheric Energy Balance",
        "author": [
            {
                "family_name": "Mbengue",
                "given_name": "Cheikh",
                "clpid": "Mbengue-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Midlatitude storm tracks shift in response to climate change and natural climate variations such as El Ni\u00f1o, but the dynamical mechanisms controlling these shifts are not well established. This paper develops an energy balance model that shows how shifts of the Hadley cell terminus and changes of the meridional energy flux out of the Hadley cell can drive shifts of storm tracks, identified as extrema of the atmospheric meridional eddy energy flux. The distance between the Hadley cell terminus and the storm tracks is primarily controlled by the energy flux out of the Hadley cell. Because tropical forcings alone can modify the Hadley cell terminus, they can also shift extratropical storm tracks, as demonstrated through simulations with an idealized GCM. Additionally, a strengthening of the meridional temperature gradient at the terminus and hence of the energy flux out of the Hadley cell can reduce the distance between the Hadley cell terminus and the storm tracks, enabling storm-track shifts that do not parallel shifts of the Hadley cell terminus. Thus, with the aid of the energy balance model and supporting GCM simulations, a closed theory of storm-track shifts emerges.",
        "doi": "10.1175/JAS-D-17-0098.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2018-03",
        "series_number": "3",
        "volume": "75",
        "issue": "3",
        "pages": "841-856"
    },
    {
        "id": "authors:rnm7e-jst84",
        "collection": "authors",
        "collection_id": "rnm7e-jst84",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20171201-113659166",
        "type": "article",
        "title": "Earth System Modeling 2.0: A Blueprint for Models That Learn From Observations and Targeted High-Resolution Simulations",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Lan",
                "given_name": "Shiwei",
                "orcid": "0000-0002-9167-3715",
                "clpid": "Lan-Shiwei"
            },
            {
                "family_name": "Stuart",
                "given_name": "Andrew",
                "orcid": "0000-0001-9091-7266",
                "clpid": "Stuart-A-M"
            },
            {
                "family_name": "Teixeira",
                "given_name": "Jo\u00e3o",
                "clpid": "Teixeira-J"
            }
        ],
        "abstract": "Climate projections continue to be marred by large uncertainties, which originate in processes that need to be parameterized, such as clouds, convection, and ecosystems. But rapid progress is now within reach. New computational tools and methods from data assimilation and machine learning make it possible to integrate global observations and local high-resolution simulations in an Earth system model (ESM) that systematically learns from both and quantifies uncertainties. Here we propose a blueprint for such an ESM. We outline how parameterization schemes can learn from global observations and targeted high-resolution simulations, for example, of clouds and convection, through matching low-order statistics between ESMs, observations, and high-resolution simulations. We illustrate learning algorithms for ESMs with a simple dynamical system that shares characteristics of the climate system; and we discuss the opportunities the proposed framework presents and the challenges that remain to realize it.",
        "doi": "10.1002/2017GL076101",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2017-12-28",
        "series_number": "24",
        "volume": "44",
        "issue": "24",
        "pages": "12396-12417"
    },
    {
        "id": "authors:kr4az-rwv97",
        "collection": "authors",
        "collection_id": "kr4az-rwv97",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20171030-144512215",
        "type": "article",
        "title": "Feedback of Atmosphere-Ocean Coupling on Shifts of the Intertropical Convergence Zone",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "It is well known that the Intertropical Convergence Zone (ITCZ) shifts in response to remote perturbations in the atmospheric energy balance, with shifts roughly in proportion to changes in the cross-equatorial atmospheric energy flux. However, atmospheric and oceanic energy fluxes in low latitudes are mechanically coupled, and the oceanic energy flux dominates the atmospheric energy flux. Here a quantitative framework is derived that shows how Ekman coupling of atmospheric and oceanic energy fluxes damps the perturbation response of the atmospheric energy flux, energy flux equator (EFE), and ITCZ. To first order, Ekman coupling alone mutes the response of EFE and ITCZ in the coupled atmosphere-ocean system by a factor \u03b3 = 1+O_0/NEI_0, where O_0 is the ocean energy uptake and NEI0 is the net energy input into the atmosphere at the equator. In the current climate in the zonal and annual mean, this factor is about \u03b3\u22483.",
        "doi": "10.1002/2017GL075817",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2017-11-28",
        "series_number": "22",
        "volume": "44",
        "issue": "22",
        "pages": "11644-11653"
    },
    {
        "id": "authors:bg10h-apy53",
        "collection": "authors",
        "collection_id": "bg10h-apy53",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170927-110506100",
        "type": "article",
        "title": "A Conceptual Model for the Response of Tropical Rainfall to Orbital Variations",
        "author": [
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Meckler",
                "given_name": "Anna Nele",
                "clpid": "Meckler-Anna-Nele"
            }
        ],
        "abstract": "Tropical rainfall to first order responds to variations in Earth's orbit through shifts of the intertropical convergence zone (ITCZ) and changes in zonally averaged rainfall intensity. Here, a conceptual model is developed that represents both processes and their response to orbital insolation variations. The model predicts the seasonal evolution of tropical rainfall between 30\u00b0S and 30\u00b0N. Insolation variations impact seasonal rainfall in two different ways: thermodynamically, leading to variations in rainfall intensity through modulation of the water vapor content of the atmosphere; and dynamically, leading to shifts of the ITCZ through modulation of the global atmospheric energy budget. Thermodynamic and dynamic effects act together to shape the annual-mean response of tropical rainfall to changes in Earth's orbit. The model successfully reproduces changes in annual-mean rainfall inferred from paleo-proxies across several glacial\u2013interglacial cycles. It illuminates how orbital precession and variations of Earth's obliquity affect tropical rainfall in distinct ways near the equator and farther away from it, with spectral signatures of precession and obliquity variations that shift with latitude. It also provides explanations for the observed different phasings of rainfall minima and maxima near the equator and away from it. For example, the model reproduces a phase shift of ~10 ka between rainfall records from caves in northern Borneo (4\u00b0N) and from China (approximately 30\u00b0N). The model suggests that such phase shifts arise through a different weighting of ITCZ shifts and variations in rainfall intensity, thus providing insight into the mechanisms that drive tropical rainfall changes on orbital time scales.",
        "doi": "10.1175/JCLI-D-16-0691.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2017-10",
        "series_number": "20",
        "volume": "30",
        "issue": "20",
        "pages": "8375-8391"
    },
    {
        "id": "authors:shz0f-9rn97",
        "collection": "authors",
        "collection_id": "shz0f-9rn97",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170831-122955794",
        "type": "article",
        "title": "Evolving perspectives on abrupt seasonal changes of the general circulation",
        "author": [
            {
                "family_name": "Lu",
                "given_name": "Jianhua",
                "clpid": "Lu-Jianhua"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Professor Duzheng YE (Tu-cheng YEH) was decades ahead of his time in proposing a model experiment to investigate whether abrupt seasonal changes of the general circulation can arise through circulation feedbacks alone, unrelated to underlying inhomogeneities at the lower boundary. Here, we introduce Professor YEH's ideas during the 1950s and 1960s on the general circulation and summarize the results and suggestions of Yeh et al. (1959) on abrupt seasonal changes. We then review recent advances in understanding abrupt seasonal changes arising from model experiments like those proposed by Yeh et al. (1959). The model experiments show that circulation feedbacks can indeed give rise to abrupt seasonal transitions. In these transitions, large-scale eddies that originate in midlatitudes and interact with the zonal mean flow and meridional overturning circulations in the tropics play central roles.",
        "doi": "10.1007/s00376-017-7068-4",
        "issn": "0256-1530",
        "publisher": "Springer",
        "publication": "Advances in Atmospheric Sciences",
        "publication_date": "2017-10",
        "series_number": "10",
        "volume": "34",
        "issue": "10",
        "pages": "1185-1194"
    },
    {
        "id": "authors:3ydhm-pcy63",
        "collection": "authors",
        "collection_id": "3ydhm-pcy63",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20171005-103437608",
        "type": "article",
        "title": "Factors controlling Hadley circulation changes from the Last Glacial Maximum to the end of the 21st century",
        "author": [
            {
                "family_name": "D'Agostino",
                "given_name": "Roberta",
                "clpid": "D'Agostino-Roberta"
            },
            {
                "family_name": "Lionello",
                "given_name": "Piero",
                "orcid": "0000-0002-0779-5681",
                "clpid": "Lionello-Piero"
            },
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The Hadley circulation (HC) extent and strength are analyzed in a wide range of simulated climates from the Last Glacial Maximum to global warming scenarios. Motivated by HC theories, we analyze how the HC is influenced by the subtropical stability, the near-surface meridional potential temperature gradient, and the tropical tropopause level. The subtropical static stability accounts for the bulk of the HC changes across the simulations. However, since it correlates strongly with global mean surface temperature, most HC changes can be attributed to global mean surface temperature changes. The HC widens as the climate warms, and it also weakens, but only robustly so in the Northern Hemisphere. On the other hand, the Southern Hemisphere strength response is uncertain, in part because subtropical static stability changes counteract meridional potential temperature gradient changes to various degrees in different models, with no consensus on the response of the latter to global warming.",
        "doi": "10.1002/2017GL074533",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2017-08-28",
        "series_number": "16",
        "volume": "44",
        "issue": "16",
        "pages": "8585-8591"
    },
    {
        "id": "authors:35mtj-33619",
        "collection": "authors",
        "collection_id": "35mtj-33619",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170629-133030446",
        "type": "article",
        "title": "Local Energetic Constraints on Walker Circulation Strength",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Levine",
                "given_name": "Xavier J.",
                "clpid": "Levine-X-J"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The weakening of tropical overturning circulations is a robust response to global warming in climate models and observations. However, there remain open questions on the causes of this change and the extent to which this weakening affects individual circulation features such as the Walker circulation. The study presents idealized GCM simulations of a Walker circulation forced by prescribed ocean heat flux convergence in a slab ocean, where the longwave opacity of the atmosphere is varied to simulate a wide range of climates. The weakening of the Walker circulation with warming results from an increase in gross moist stability (GMS), a measure of the tropospheric moist static energy (MSE) stratification, which provides an effective static stability for tropical circulations. Baroclinic mode theory is used to determine changes in GMS in terms of the tropical-mean profiles of temperature and MSE. The GMS increases with warming, owing primarily to the rise in tropopause height, decreasing the sensitivity of the Walker circulation to zonally anomalous net energy input. In the absence of large changes in net energy input, this results in a rapid weakening of the Walker circulation with global warming.",
        "doi": "10.1175/JAS-D-16-0219.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2017-06",
        "series_number": "6",
        "volume": "74",
        "issue": "6",
        "pages": "1907-1922"
    },
    {
        "id": "authors:8s9nh-z3s80",
        "collection": "authors",
        "collection_id": "8s9nh-z3s80",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170501-080154912",
        "type": "article",
        "title": "Numerics and subgrid-scale modeling in large eddy simulations of stratocumulus clouds",
        "author": [
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            },
            {
                "family_name": "Mishra",
                "given_name": "Siddhartha",
                "orcid": "0000-0002-2665-5385",
                "clpid": "Mishra-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-C-M"
            },
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            }
        ],
        "abstract": "Stratocumulus clouds are the most common type of boundary layer cloud; their radiative effects strongly modulate climate. Large eddy simulations (LES) of stratocumulus clouds often struggle to maintain fidelity to observations because of the sharp gradients occurring at the entrainment interfacial layer at the cloud top. The challenge posed to LES by stratocumulus clouds is evident in the wide range of solutions found in the LES intercomparison based on the DYCOMS-II field campaign, where simulated liquid water paths for identical initial and boundary conditions varied by a factor of nearly 12. Here we revisit the DYCOMS-II RF01 case and show that the wide range of previous LES results can be realized in a single LES code by varying only the numerical treatment of the equations of motion and the nature of subgrid-scale (SGS) closures. The simulations that maintain the greatest fidelity to DYCOMS-II observations are identified. The results show that using weighted essentially non-oscillatory (WENO) numerics for all resolved advective terms and no explicit SGS closure consistently produces the highest-fidelity simulations. This suggests that the numerical dissipation inherent in WENO schemes functions as a high-quality, implicit SGS closure for this stratocumulus case. Conversely, using oscillatory centered difference numerical schemes for momentum advection, WENO numerics for scalars, and explicitly modeled SGS fluxes consistently produces the lowest-fidelity simulations. We attribute this to the production of anomalously large SGS fluxes near the cloud tops through the interaction of numerical error in the momentum field with the scalar SGS model.",
        "doi": "10.1002/2016MS000778",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2017-06",
        "series_number": "2",
        "volume": "9",
        "issue": "2",
        "pages": "1342-1365"
    },
    {
        "id": "authors:ryazh-58p91",
        "collection": "authors",
        "collection_id": "ryazh-58p91",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20181218-154520884",
        "type": "article",
        "title": "Large-eddy simulation of subtropical cloud-topped boundary layers: 2. Cloud response to climate change",
        "author": [
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Teixeira",
                "given_name": "Jo\u00e3o",
                "clpid": "Teixeira-J"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            }
        ],
        "abstract": "How subtropical marine boundary layer (MBL) clouds respond to warming is investigated using large\u2010eddy simulations (LES) of a wide range of warmer climates, with CO_2 concentrations elevated by factors 2\u201316. In LES coupled to a slab ocean with interactive sea surface temperatures (SST), the surface latent heat flux (LHF) is constrained by the surface energy balance and only strengthens modestly under warming. Consequently, the MBL in warmer climates is shallower than in corresponding fixed\u2010SST LES, in which LHF strengthens excessively and the MBL typically deepens. The inferred shortwave (SW) cloud feedback with a closed energy balance is weakly positive for cumulus clouds. It is more strongly positive for stratocumulus clouds, with a magnitude that increases with warming. Stratocumulus clouds generally break up above 6 K to 9 K warming, or above a four to eightfold increase in CO_2 concentrations. This occurs because the MBL mixing driven by cloud\u2010top longwave (LW) cooling weakens as the LW opacity of the free troposphere increases. The stratocumulus breakup triggers an abrupt and large SST increase and MBL deepening, which cannot occur in fixed\u2010SST experiments. SW cloud radiative effects generally weaken while the lower\u2010tropospheric stability increases under warming\u2014the reverse of their empirical relation in the present climate. The MBL is deeper and stratocumulus persists into warmer climates if large\u2010scale subsidence decreases as the climate warms. The contrasts between experiments with interactive SST and fixed SST highlight the importance of a closed surface energy balance for obtaining realizable responses of MBL clouds to warming.",
        "doi": "10.1002/2016ms000804",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2017-03",
        "series_number": "1",
        "volume": "9",
        "issue": "1",
        "pages": "19-38"
    },
    {
        "id": "authors:pm2eq-4qn31",
        "collection": "authors",
        "collection_id": "pm2eq-4qn31",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170216-124419096",
        "type": "article",
        "title": "Storm-Track Shifts under Climate Change: Toward a Mechanistic Understanding Using Baroclinic Mean Available Potential Energy",
        "author": [
            {
                "family_name": "Mbengue",
                "given_name": "Cheikh",
                "clpid": "Mbengue-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Zonal-mean storm-track shifts in response to perturbations in climate occur even in idealized simulations of dry atmospheres with axisymmetric forcing. Nonetheless, a generally accepted theory of the mechanisms controlling the storm-track shifts is still lacking. Here, mean available potential energy (MAPE), a general measure of baroclinicity that is proportional to the square of the Eady growth rate, is used to understand storm-track shifts. It is demonstrated that, in dry atmospheres, the eddy kinetic energy (EKE) in a storm track is linearly related to the mean available potential energy, relative to a local reference state, and that maxima of the two are generally collocated in latitude. Changes in MAPE with climate are then decomposed into components. It is shown that in simulations of dry atmospheres, changes in the latitude of maximum MAPE are dominated by changes in near-surface meridional temperature gradients. By contrast, changes in the magnitude of MAPE are primarily determined by changes in static stability and in the depth of the troposphere. A theory of storm-track shifts may build upon these findings and primarily needs to explain changes in near-surface meridional temperature gradients. The terminus of the Hadley circulation often shifts in tandem with storm tracks and is hypothesized to play an important role in triggering the storm-track shifts seen in this idealized dry context, especially in simulations where increases only in the convective static stability in the deep tropics suffice to shift storm tracks poleward.",
        "doi": "10.1175/JAS-D-15-0267.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2017-01",
        "series_number": "1",
        "volume": "74",
        "issue": "1",
        "pages": "93-110"
    },
    {
        "id": "authors:j6bp1-f2r38",
        "collection": "authors",
        "collection_id": "j6bp1-f2r38",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-083859656",
        "type": "article",
        "title": "The organization of Jupiter's upper tropospheric temperature structure and its evolution, 1996\u20131997",
        "author": [
            {
                "family_name": "Fisher",
                "given_name": "Brendan M.",
                "clpid": "Fisher-B-M"
            },
            {
                "family_name": "Orton",
                "given_name": "Glenn S.",
                "orcid": "0000-0001-7871-2823",
                "clpid": "Orton-G-S"
            },
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Ressler",
                "given_name": "Michael E.",
                "clpid": "Ressler-M-E"
            },
            {
                "family_name": "Hoffmann",
                "given_name": "William F.",
                "clpid": "Hoffmann-W-F"
            }
        ],
        "abstract": "High signal-to-noise images of Jupiter were made at wavelengths between 13.2 and 22.8 \u00b5m in five separate observing runs between 1996 June and 1997 November at the NASA Infrared Telescope Facility. Maps of Jupiter's upper-tropospheric temperatures at pressures of 100 and 400 mbar were made from these images. We use the relatively frequent, well sampled data sets to examine in detail the short-term evolution of the temperature structure. Our 2\u20136 month sampling periods demonstrate that the longitudinal temperature structures evolve significantly in these short periods and exhibit wave features. Using a three-dimensional general circulation model simulation of Jupiter's upper atmosphere, we show that the thermal structures are consistent with convectively generated Rossby waves that propagate upward from the lower to the upper atmosphere.",
        "doi": "10.1016/j.icarus.2016.07.016",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2016-12",
        "volume": "280",
        "pages": "268-277"
    },
    {
        "id": "authors:2h107-g8064",
        "collection": "authors",
        "collection_id": "2h107-g8064",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20181218-155745542",
        "type": "article",
        "title": "Large-eddy simulation of subtropical cloud\u2010topped boundary layers: 1. A forcing framework with closed surface energy balance",
        "author": [
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Teixeira",
                "given_name": "Jo\u00e3o",
                "clpid": "Teixeira-J"
            },
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            }
        ],
        "abstract": "Large\u2010eddy simulation (LES) of clouds has the potential to resolve a central question in climate dynamics, namely, how subtropical marine boundary layer (MBL) clouds respond to global warming. However, large\u2010scale processes need to be prescribed or represented parameterically in the limited\u2010area LES domains. It is important that the representation of large\u2010scale processes satisfies constraints such as a closed energy balance in a manner that is realizable under climate change. For example, LES with fixed sea surface temperatures usually do not close the surface energy balance, potentially leading to spurious surface fluxes and cloud responses to climate change. Here a framework of forcing LES of subtropical MBL clouds is presented that enforces a closed surface energy balance by coupling atmospheric LES to an ocean mixed layer with a sea surface temperature (SST) that depends on radiative fluxes and sensible and latent heat fluxes at the surface. A variety of subtropical MBL cloud regimes (stratocumulus, cumulus, and stratocumulus over cumulus) are simulated successfully within this framework. However, unlike in conventional frameworks with fixed SST, feedbacks between cloud cover and SST arise, which can lead to sudden transitions between cloud regimes (e.g., stratocumulus to cumulus) as forcing parameters are varied. The simulations validate this framework for studies of MBL clouds and establish its usefulness for studies of how the clouds respond to climate change.",
        "doi": "10.1002/2016MS000655",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2016-12",
        "series_number": "4",
        "volume": "8",
        "issue": "4",
        "pages": "1565-1585"
    },
    {
        "id": "authors:j06ay-zcc32",
        "collection": "authors",
        "collection_id": "j06ay-zcc32",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20170106-154835521",
        "type": "article",
        "title": "Narrowing of the ITCZ in a warming climate: Physical mechanisms",
        "author": [
            {
                "family_name": "Byrne",
                "given_name": "Michael P.",
                "clpid": "Byrne-M-P"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The Intertropical Convergence Zone (ITCZ) narrows in response to global warming in both observations and climate models. However, a physical understanding of this narrowing is lacking. Here we show that the narrowing of the ITCZ in simulations of future climate is related to changes in the moist static energy (MSE) budget. MSE advection by the mean circulation and MSE divergence by transient eddies tend to narrow the ITCZ, while changes in net energy input to the atmosphere and the gross moist stability tend to widen the ITCZ. The narrowing tendency arises because the meridional MSE gradient strengthens with warming, whereas the largest widening tendency is due to increasing shortwave heating of the atmosphere. The magnitude of the ITCZ narrowing depends strongly on the gross moist stability and clouds, emphasizing the need to better understand these fundamental processes in the tropical atmosphere.",
        "doi": "10.1002/2016GL070396",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2016-11-16",
        "series_number": "21",
        "volume": "43",
        "issue": "21",
        "pages": "11350-11357"
    },
    {
        "id": "authors:js9mr-hah98",
        "collection": "authors",
        "collection_id": "js9mr-hah98",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-151837626",
        "type": "article",
        "title": "Seasonal and Interannual Variations of the Energy Flux Equator and ITCZ. Part II: Zonally Varying Shifts of the ITCZ",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The ITCZ lies at the ascending branch of the tropical meridional overturning circulation, where near-surface meridional mass fluxes vanish. Near the ITCZ, column-integrated energy fluxes vanish, forming an atmospheric energy flux equator (EFE). This paper extends existing approximations relating the ITCZ position and EFE to the atmospheric energy budget by allowing for zonal variations. The resulting relations are tested using reanalysis data for 1979\u20132014. The zonally varying EFE is found as the latitude where the meridional component of the divergent atmospheric energy transport (AET) vanishes. A Taylor expansion of the AET around the equator relates the ITCZ position to derivatives of the AET. To a first order, the ITCZ position is proportional to the divergent AET across the equator; it is inversely proportional to the local atmospheric net energy input (NEI) that consists of the net energy fluxes at the surface, at the top of the atmosphere, and zonally across longitudes. The first-order approximation captures the seasonal migrations of the ITCZ in the African, Asian, and Atlantic sectors. In the eastern Pacific, a third-order approximation captures the bifurcation from single- to double-ITCZ states that occurs during boreal spring. In contrast to linear EFE theory, during boreal winter in the eastern Pacific, northward cross-equatorial AET goes along with an ITCZ north of the equator. EFE and ITCZ variations driven by ENSO are characterized by an equatorward (poleward) shift in the Pacific during El Ni\u00f1o (La Ni\u00f1a) episodes, which are associated with variations in equatorial ocean energy uptake.",
        "doi": "10.1175/JCLI-D-15-0710.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-10",
        "series_number": "20",
        "volume": "29",
        "issue": "20",
        "pages": "7281-7293"
    },
    {
        "id": "authors:x0ana-6ry45",
        "collection": "authors",
        "collection_id": "x0ana-6ry45",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-152816638",
        "type": "article",
        "title": "Constraints on Climate Sensitivity from Space-Based Measurements of Low-Cloud Reflection",
        "author": [
            {
                "family_name": "Brient",
                "given_name": "Florent",
                "clpid": "Brient-Florent"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Physical uncertainties in global-warming projections are dominated by uncertainties about how the fraction of incoming shortwave radiation that clouds reflect will change as greenhouse gas concentrations rise. Differences in the shortwave reflection by low clouds over tropical oceans alone account for more than half of the variance of the equilibrium climate sensitivity (ECS) among climate models, which ranges from 2.1 to 4.7 K. Space-based measurements now provide an opportunity to assess how well models reproduce temporal variations of this shortwave reflection on seasonal to interannual time scales. Here such space-based measurements are used to show that shortwave reflection by low clouds over tropical oceans decreases robustly when the underlying surface warms, for example, by \u2212(0.96 \u00b1 0.22)% K^(\u22121) (90% confidence level) for deseasonalized variations. Additionally, the temporal covariance of low-cloud reflection with temperature in historical simulations with current climate models correlates strongly (r = \u22120.67) with the models' ECS. Therefore, measurements of temporal low-cloud variations can be used to constrain ECS estimates based on climate models. An information-theoretic weighting of climate models by how well they reproduce the measured deseasonalized covariance of shortwave cloud reflection with temperature yields a most likely ECS estimate around 4.0 K; an ECS below 2.3 K becomes very unlikely (90% confidence).",
        "doi": "10.1175/JCLI-D-15-0897.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-08",
        "series_number": "16",
        "volume": "29",
        "issue": "16",
        "pages": "5821-5835"
    },
    {
        "id": "authors:1m721-4b096",
        "collection": "authors",
        "collection_id": "1m721-4b096",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-152157215",
        "type": "article",
        "title": "Relation of the double-ITCZ bias to the atmospheric energy budget in climate models",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Brient",
                "given_name": "Florent",
                "clpid": "Brient-Florent"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            }
        ],
        "abstract": "We examine how tropical zonal mean precipitation biases in current climate models relate to the atmospheric energy budget. Both hemispherically symmetric and antisymmetric tropical precipitation biases contribute to the well-known double-Intertropical Convergence Zone (ITCZ) bias; however, they have distinct signatures in the energy budget. Hemispherically symmetric biases in tropical precipitation are proportional to biases in the equatorial net energy input; hemispherically antisymmetric biases are proportional to the atmospheric energy transport across the equator. Both relations can be understood within the framework of recently developed theories. Atmospheric net energy input biases in the deep tropics shape both the symmetric and antisymmetric components of the double-ITCZ bias. Potential causes of these energetic biases and their variation across climate models are discussed.",
        "doi": "10.1002/2016GL069465",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2016-07-28",
        "series_number": "14",
        "volume": "43",
        "issue": "14",
        "pages": "7670-7677"
    },
    {
        "id": "authors:t5tnj-a9s10",
        "collection": "authors",
        "collection_id": "t5tnj-a9s10",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160720-153809020",
        "type": "article",
        "title": "Contrasting responses to orbital precession on Titan and Earth",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Earth and Titan exhibit contrasting atmospheric responses to orbital precession. On Earth, most (water) precipitation falls in low latitudes, and precipitation is enhanced in a hemisphere when perihelion occurs in that hemisphere's summer. On Titan, most (methane) precipitation falls in high latitudes, and precipitation is enhanced in a hemisphere when aphelion occurs in that hemisphere's summer. We use a Titan general circulation model to elucidate the dynamical reasons for these different responses to orbital precession. They arise primarily because of the different diurnal rotation rates of Titan and Earth. The slower rotation rate of Titan leads to wider Hadley cells that transport moisture into polar regions. Changes in the length of summer, rather than in the intensity of summer insolation as in Earth's tropics, then dominate the precession response of the hydrologic cycle.",
        "doi": "10.1002/2016GL070065",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2016-07-28",
        "series_number": "14",
        "volume": "43",
        "issue": "14",
        "pages": "7774-7780"
    },
    {
        "id": "authors:nj7j5-1ta92",
        "collection": "authors",
        "collection_id": "nj7j5-1ta92",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160715-154332491",
        "type": "article",
        "title": "Energetic Constraints on the Width of the Intertropical Convergence Zone",
        "author": [
            {
                "family_name": "Byrne",
                "given_name": "Michael P.",
                "clpid": "Byrne-M-P"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The intertropical convergence zone (ITCZ) has been the focus of considerable research in recent years, with much of this work concerned with how the latitude of maximum tropical precipitation responds to natural climate variability and to radiative forcing. The width of the ITCZ, however, has received little attention despite its importance for regional climate and for understanding the general circulation of the atmosphere. This paper investigates the ITCZ width in simulations with an idealized general circulation model over a wide range of climates. The ITCZ, defined as the tropical region where there is time-mean ascent, displays rich behavior as the climate varies, widening with warming in cool climates, narrowing in temperate climates, and maintaining a relatively constant width in hot climates. The mass and energy budgets of the Hadley circulation are used to derive expressions for the area of the ITCZ relative to the area of the neighboring descent region, and for the sensitivity of the ITCZ area to changes in climate. The ITCZ width depends primarily on four quantities: the net energy input to the tropical atmosphere, the advection of moist static energy by the Hadley circulation, the transport of moist static energy by transient eddies, and the gross moist stability. Different processes are important for the ITCZ width in different climates, with changes in gross moist stability generally having a weak influence relative to the other processes. The results are likely to be useful for analyzing the ITCZ width in complex climate models and for understanding past and future climate change in the tropics.",
        "doi": "10.1175/JCLI-D-15-0767.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-07",
        "series_number": "13",
        "volume": "29",
        "issue": "13",
        "pages": "4709-4721"
    },
    {
        "id": "authors:kprn6-rdk40",
        "collection": "authors",
        "collection_id": "kprn6-rdk40",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-135131589",
        "type": "article",
        "title": "Shallowness of tropical low clouds as a predictor of climate models' response to warming",
        "author": [
            {
                "family_name": "Brient",
                "given_name": "Florent",
                "clpid": "Brient-Florent"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Bony",
                "given_name": "Sandrine",
                "clpid": "Bony-Sandrine"
            },
            {
                "family_name": "Qu",
                "given_name": "Xin",
                "clpid": "Qu-Xin"
            },
            {
                "family_name": "Hall",
                "given_name": "Alex",
                "clpid": "Hall-Alex"
            }
        ],
        "abstract": "How tropical low clouds change with climate remains the dominant source of uncertainty in global warming projections. An analysis of an ensemble of CMIP5 climate models reveals that a significant part of the spread in the models' climate sensitivity can be accounted by differences in the climatological shallowness of tropical low clouds in weak-subsidence regimes: models with shallower low clouds in weak-subsidence regimes tend to have a higher climate sensitivity than models with deeper low clouds. The dynamical mechanisms responsible for the model differences are analyzed. Competing effects of parameterized boundary-layer turbulence and shallow convection are found to be essential. Boundary-layer turbulence and shallow convection are typically represented by distinct parameterization schemes in current models\u2014parameterization schemes that often produce opposing effects on low clouds. Convective drying of the boundary layer tends to deepen low clouds and reduce the cloud fraction at the lowest levels; turbulent moistening tends to make low clouds more shallow but affects the low-cloud fraction less. The relative importance different models assign to these opposing mechanisms contributes to the spread of the climatological shallowness of low clouds and thus to the spread of low-cloud changes under global warming.",
        "doi": "10.1007/s00382-015-2846-0",
        "issn": "0930-7575",
        "publisher": "Springer",
        "publication": "Climate Dynamics",
        "publication_date": "2016-07",
        "series_number": "1-2",
        "volume": "47",
        "issue": "1-2",
        "pages": "433-449"
    },
    {
        "id": "authors:j542g-8m452",
        "collection": "authors",
        "collection_id": "j542g-8m452",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160715-153714338",
        "type": "article",
        "title": "Thermodynamic and dynamic controls on changes in the zonally anomalous hydrological cycle",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Byrne",
                "given_name": "Michael P.",
                "clpid": "Byrne-M-P"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The wet gets wetter, dry gets drier paradigm explains the expected moistening of the extratropics and drying of the subtropics as the atmospheric moisture content increases with global warming. Here we show, using precipitation minus evaporation (P \u2212 E) data from climate models, that it cannot be extended to apply regionally to deviations from the zonal mean. Wet and dry zones shift substantially in response to shifts in the stationary-eddy circulations that cause them. Additionally, atmospheric circulation changes lead to a smaller increase in the zonal variance of P \u2212 E than would be expected from atmospheric moistening alone. The P \u2212 E variance change can be split into dynamic and thermodynamic components through an analysis of the atmospheric moisture budget. This reveals that a weakening of stationary-eddy circulations and changes in the zonal variation of transient-eddy moisture fluxes moderate the strengthening of the zonally anomalous hydrological cycle with global warming.",
        "doi": "10.1002/2016GL068418",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2016-05-16",
        "series_number": "9",
        "volume": "43",
        "issue": "9",
        "pages": "4640-4649"
    },
    {
        "id": "authors:mhn4y-tx252",
        "collection": "authors",
        "collection_id": "mhn4y-tx252",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160601-080822648",
        "type": "article",
        "title": "How Stationary Eddies Shape Changes in the Hydrological Cycle: Zonally Asymmetric Experiments in an Idealized GCM",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Stationary and low-frequency Rossby waves are the primary drivers of extratropical weather variations on monthly and longer time scales. They take the form of persistent highs and lows, which, for example, shape subtropical dry zones and guide extratropical storms. More generally, stationary-eddy circulations, including zonally anomalous tropical overturning circulations, set up large zonal variations in net precipitation (precipitation minus evaporation, P \u2212 E). This paper investigates the response of stationary eddies and the zonally asymmetric hydrological cycle to global warming in an idealized GCM, simulating a wide range of climates by varying longwave absorption. The stationary eddies are forced by two idealized zonal asymmetries: a midlatitude Gaussian mountain and an equatorial ocean heat source. Associated with changes in stationary eddies are changes in the zonal variation of the hydrological cycle. Particularly in the subtropics, these simulations show a nearly constant or decreasing amplitude of the zonally anomalous hydrological cycle in climates warmer than modern despite the wet gets wetter, dry gets drier effect associated with increasing atmospheric moisture content. An approximation for zonally anomalous P \u2212 E, based on zonal-mean surface specific humidity and stationary-eddy vertical motion, disentangles the roles of thermodynamic and dynamic changes. The approximation shows that changes in the zonally asymmetric hydrological cycle are predominantly controlled by changes in lower-tropospheric vertical motion in stationary eddies.",
        "doi": "10.1175/JCLI-D-15-0781.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-05",
        "series_number": "9",
        "volume": "29",
        "issue": "9",
        "pages": "3161-3179"
    },
    {
        "id": "authors:qf6j2-nds93",
        "collection": "authors",
        "collection_id": "qf6j2-nds93",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160601-095902123",
        "type": "article",
        "title": "Seasonal and Interannual Variations of the Energy Flux Equator and ITCZ. Part I: Zonally Averaged ITCZ Position",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "In the zonal mean, the ITCZ lies at the foot of the ascending branch of the tropical mean meridional circulation, close to where the near-surface meridional mass flux vanishes. The ITCZ also lies near the energy flux equator (EFE), where the column-integrated meridional energy flux vanishes. This latter observation makes it possible to relate the ITCZ position to the energy balance, specifically the atmospheric net energy input near the equator and the cross-equatorial energy flux. Here the validity of the resulting relations between the ITCZ position and energetic quantities is examined with reanalysis data for the years 1979\u20132014. In the reanalysis data, the EFE and ITCZ position indeed covary on time scales of seasons and longer. Consistent with theory, the ITCZ position is proportional to the cross-equatorial atmospheric energy flux and inversely proportional to atmospheric net energy input at the equator. Variations of the cross-equatorial energy flux dominate seasonal variations of the ITCZ position. By contrast, variations of the equatorial net energy input, driven by ocean energy uptake variations, dominate interannual variations of the ITCZ position (e.g., those associated with ENSO).",
        "doi": "10.1175/JCLI-D-15-0512.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-04-19",
        "series_number": "9",
        "volume": "29",
        "issue": "9",
        "pages": "3219-3230"
    },
    {
        "id": "authors:tdj6h-mm568",
        "collection": "authors",
        "collection_id": "tdj6h-mm568",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160520-084733761",
        "type": "article",
        "title": "The Equatorial Energy Balance, ITCZ Position, and Double-ITCZ Bifurcations",
        "author": [
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The intertropical convergence zone (ITCZ) migrates north\u2013south on seasonal and longer time scales. Previous studies have shown that the zonal-mean ITCZ displacement off the equator is negatively correlated with the energy flux across the equator; when the ITCZ lies in the Northern Hemisphere, energy flows southward across the equator, and vice versa. The hemisphere that exports energy across the equator is the hemisphere with more net energy input, and it is usually the warmer hemisphere. But states with a double ITCZ straddling the equator also occur, for example, seasonally over the eastern Pacific and frequently in climate models. Here it is shown how the ITCZ position is connected to the energy balance near the equator in a broad range of circumstances, including states with single and double ITCZs. Taylor expansion of the variation of the meridional energy flux around the equator leads to the conclusion that for large positive net energy input into the equatorial atmosphere, the ITCZ position depends linearly on the cross-equatorial energy flux. For small positive equatorial net energy input, the dependence of the ITCZ position on the cross-equatorial energy flux weakens to the third root. When the equatorial net energy input or its curvature become negative, a bifurcation to double-ITCZ states occurs. Simulations with an idealized aquaplanet general circulation model (GCM) confirm the quantitative adequacy of these relations. The results provide a framework for assessing and understanding causes of common climate model biases and for interpreting tropical precipitation changes, such as those evident in records of climates of the past.",
        "doi": "10.1175/JCLI-D-15-0328.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2016-04",
        "series_number": "8",
        "volume": "29",
        "issue": "8",
        "pages": "2997-3013"
    },
    {
        "id": "authors:5dzzw-v0204",
        "collection": "authors",
        "collection_id": "5dzzw-v0204",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160415-082349241",
        "type": "article",
        "title": "Cumulant expansions for atmospheric flows",
        "author": [
            {
                "family_name": "Ait-Chaalal",
                "given_name": "Farid",
                "clpid": "Ait-Chaalal-F"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Meyer",
                "given_name": "Bettina",
                "clpid": "Meyer-B"
            },
            {
                "family_name": "Marston",
                "given_name": "J. B.",
                "clpid": "Marston-J-B"
            }
        ],
        "abstract": "Atmospheric flows are governed by the equations of fluid dynamics. These equations are nonlinear, and consequently the hierarchy of cumulant equations is not closed. But because atmospheric flows are inhomogeneous and anisotropic, the nonlinearity may manifest itself only weakly through interactions of nontrivial mean fields with disturbances such as thermals or eddies. In such situations, truncations of the hierarchy of cumulant equations hold promise as a closure strategy. Here we show how truncations at second order can be used to model and elucidate the dynamics of turbulent atmospheric flows. Two examples are considered. First, we study the growth of a dry convective boundary layer, which is heated from below, leading to turbulent upward energy transport and growth of the boundary layer. We demonstrate that a quasilinear truncation of the equations of motion, in which interactions of disturbances among each other are neglected but interactions with mean fields are taken into account, can capture the growth of the convective boundary layer. However, it does not capture important turbulent transport terms in the turbulence kinetic energy budget. Second, we study the evolution of two-dimensional large-scale waves, which are representative of waves seen in Earth's upper atmosphere. We demonstrate that a cumulant expansion truncated at second order (CE2) can capture the evolution of such waves and their nonlinear interaction with the mean flow in some circumstances, for example, when the wave amplitude is small enough or the planetary rotation rate is large enough. However, CE2 fails to capture the flow evolution when strongly nonlinear eddy\u2013eddy interactions that generate small-scale filaments in surf zones around critical layers become important. Higher-order closures can capture these missing interactions. The results point to new ways in which the dynamics of turbulent boundary layers may be represented in climate models, and they illustrate different classes of nonlinear processes that can control wave dissipation and angular momentum fluxes in the upper troposphere.",
        "doi": "10.1088/1367-2630/18/2/025019",
        "issn": "1367-2630",
        "publisher": "IOP",
        "publication": "New Journal of Physics",
        "publication_date": "2016-02",
        "series_number": "2",
        "volume": "18",
        "issue": "2",
        "pages": "Art. No. 025019"
    },
    {
        "id": "authors:jdg6w-b0t15",
        "collection": "authors",
        "collection_id": "jdg6w-b0t15",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20151130-112437219",
        "type": "article",
        "title": "Superrotation in Terrestrial Atmospheres",
        "author": [
            {
                "family_name": "Laraia",
                "given_name": "Anne L.",
                "clpid": "Laraia-A-L"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Atmospheric superrotation with prograde equatorial winds and an equatorial angular momentum maximum is ubiquitous in planetary atmospheres. It is clear that eddy fluxes of angular momentum toward the equator are necessary to generate it. But under what conditions superrotation arises has remained unclear. This paper presents simulations and a scaling theory that establish conditions under which superrotation occurs in terrestrial atmospheres. Whether superrotation arises depends on the relative importance of factors that favor or disfavor superrotation. Convection preferentially generates Rossby waves near the equator, where the Rossby number is O(1). Since the Rossby waves transport angular momentum toward their source regions, this favors superrotation. Meridional temperature gradients preferentially lead to baroclinic instability and wave generation away from the equator. Eddy transport of angular momentum toward the baroclinic source region implies transport out of low latitudes, which disfavors superrotation. Simulations with an idealized GCM show that superrotation tends to arise when the equatorial convective generation of wave activity and its associated eddy angular momentum flux convergence exceed the baroclinic eddy angular momentum flux divergence. Convective and baroclinic wave activity generation is related through scaling arguments to mean-flow properties, such as planetary rotation rates and meridional temperature gradients. The scaling arguments show, for example, that superrotation is favored when the off-equatorial baroclinicity and planetary rotation rates are low, as they are, for example, on Venus. Similarly, superrotation is favored when the convective heating strengthens, which may account for the superrotation seen in extreme global warming simulations.",
        "doi": "10.1175/JAS-D-15-0030.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2015-11",
        "series_number": "11",
        "volume": "72",
        "issue": "11",
        "pages": "4281-4296"
    },
    {
        "id": "authors:p3jd8-cfx78",
        "collection": "authors",
        "collection_id": "p3jd8-cfx78",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20151112-153703322",
        "type": "article",
        "title": "Large-eddy simulation in an anelastic framework with closed water and entropy balances",
        "author": [
            {
                "family_name": "Pressel",
                "given_name": "Kyle G.",
                "orcid": "0000-0002-4538-3055",
                "clpid": "Pressel-K-G"
            },
            {
                "family_name": "Kaul",
                "given_name": "Colleen M.",
                "orcid": "0000-0002-4462-0987",
                "clpid": "Kaul-C-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Tan",
                "given_name": "Zhihong",
                "orcid": "0000-0002-7422-3317",
                "clpid": "Tan-Zhihong"
            },
            {
                "family_name": "Mishra",
                "given_name": "Siddhartha",
                "orcid": "0000-0002-2665-5385",
                "clpid": "Mishra-S"
            }
        ],
        "abstract": "A large-eddy simulation (LES) framework is developed for simulating the dynamics of clouds and boundary layers with closed water and entropy balances. The framework is based on the anelastic equations in a formulation that remains accurate for deep convection. As prognostic variables, it uses total water and entropy, which are conserved in adiabatic and reversible processes, including reversible phase changes of water. This has numerical advantages for modeling clouds, in which reversible phase changes of water occur frequently. The equations of motion are discretized using higher-order weighted essentially nonoscillatory (WENO) discretization schemes with strong stability preserving time stepping. Numerical tests demonstrate that the WENO schemes yield simulations superior to centered schemes, even when the WENO schemes are used at coarser resolution. The framework is implemented in a new LES code written in Python and Cython, which makes the code transparent and easy to use for a wide user group.",
        "doi": "10.1002/2015MS000496",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2015-09",
        "series_number": "3",
        "volume": "7",
        "issue": "3",
        "pages": "1425-1456"
    },
    {
        "id": "authors:va186-4bh79",
        "collection": "authors",
        "collection_id": "va186-4bh79",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150806-143422294",
        "type": "article",
        "title": "Baroclinic Eddies and the Extent of the Hadley Circulation: An Idealized GCM Study",
        "author": [
            {
                "family_name": "Levine",
                "given_name": "Xavier J.",
                "clpid": "Levine-X-J"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The Hadley circulation has widened over the past 30 years. This widening has been qualitatively reproduced in general circulation model (GCM) simulations of a warming climate. Comprehensive GCM studies suggest this widening may be caused by a poleward shift in baroclinic eddy activity. Yet the limited amplitude of the climate change signals analyzed so far precludes a quantitative comparison with theories.\n\nThis study uses two idealized GCMs, one with and one without an active hydrologic cycle, to investigate changes in the extent of the Hadley circulation over a wide range of climates. The climates span global-mean temperatures from 243 to 385 K and equator-to-pole temperature contrasts from 12 to 100 K. Baroclinic eddies control the extent of the Hadley circulation across most of these climates. A supercriticality criterion that quantifies the depth of baroclinic eddies relative to that of the troposphere turns out to be a good indicator of where baroclinic eddies become deep enough to terminate the Hadley circulation. The supercriticality depends on meridional temperature gradients and an effective stability that accounts for the effect of convective heating on baroclinic eddies.\n\nAs the equator-to-pole temperature contrast weakens or the convective static stability increases, convective heating increasingly influences the thermal stratification of the troposphere and the supercriticality. Consistent with the supercriticality criterion, the Hadley circulation contracts as meridional temperature gradients increase, and it widens as the effective static stability increases. The former occurs during El Ni\u00f1o and may account for the observed Hadley circulation contraction then; the latter occurs during global warming.",
        "doi": "10.1175/JAS-D-14-0152.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2015-07",
        "series_number": "7",
        "volume": "72",
        "issue": "7",
        "pages": "2744-2761"
    },
    {
        "id": "authors:r5fxh-n9y17",
        "collection": "authors",
        "collection_id": "r5fxh-n9y17",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150724-110437816",
        "type": "article",
        "title": "Stationary Eddies and the Zonal Asymmetry of Net Precipitation and Ocean Freshwater Forcing",
        "author": [
            {
                "family_name": "Wills",
                "given_name": "Robert C.",
                "orcid": "0000-0002-7776-2076",
                "clpid": "Wills-R-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Transport of water vapor in the atmosphere generates substantial spatial variability of net precipitation\n(precipitation minus evaporation). Over half of the total spatial variability in annual-mean net precipitation is\naccounted for by deviations from the zonal mean. Over land, these regional differences determine differences in\nsurface water availability. Over oceans, they account, for example, for the Pacific\u2013Atlantic difference in sea\nsurface salinity, with implications for the deep overturning circulation. This study analyzes the atmospheric-water\nbudget in reanalyses from ERA-Interim and MERRA, to investigate which physical balances lead to zonal\nvariation in net precipitation. It is found that the leading-order contribution is zonal variation in stationary-eddy\nvertical motion. Transient eddies modify the pattern of zonally anomalous net precipitation by moving moisture\nfrom the subtropical and tropical oceans onto land and poleward across the Northern Hemisphere storm tracks.\nZonal variation in specific humidity and stationary-eddy horizontal advection play a secondary role. The dynamics\nleading to net precipitation via vertical motion in stationary eddies can be understood from a lower-tropospheric\nvorticity budget. The large-scale variations of vertical motion are primarily described by Sverdrup\nbalance and Ekman pumping, with some modification by transient eddies. These results suggest that it is important\nto understand changes in stationary eddies and their influence on the zonal variation of transient eddy\nfluxes, in order to understand regional changes in net precipitation. They highlight the relative importance of\ndifferent atmospheric mechanisms for the freshwater forcing of the North Pacific and North Atlantic.",
        "doi": "10.1175/JCLI-D-14-00573.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2015-07",
        "series_number": "13",
        "volume": "28",
        "issue": "13",
        "pages": "5115-5133"
    },
    {
        "id": "authors:3kj0q-w2m19",
        "collection": "authors",
        "collection_id": "3kj0q-w2m19",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150522-100044286",
        "type": "article",
        "title": "Interannual Variability in the Large-Scale Dynamics of the South Asian Summer Monsoon",
        "author": [
            {
                "family_name": "Walker",
                "given_name": "Jennifer M.",
                "clpid": "Walker-J-M"
            },
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "This study identifies coherent and robust large-scale atmospheric patterns of interannual variability of the South Asian summer monsoon (SASM) in observational data. A decomposition of the water vapor budget into dynamic and thermodynamic components shows that interannual variability of SASM net precipitation (P \u2212 E) is primarily caused by variations in winds rather than in moisture. Linear regression analyses reveal that strong monsoons are distinguished from weak monsoons by a northward expansion of the cross-equatorial monsoonal circulation, with increased precipitation in the ascending branch. Interestingly, and in disagreement with the view of monsoons as large-scale sea-breeze circulations, strong monsoons are associated with a decreased meridional gradient in the near-surface atmospheric temperature in the SASM region. Teleconnections exist from the SASM region to the Southern Hemisphere, whose midlatitude poleward eddy energy flux correlates with monsoon strength. Possible implications of these teleconnection patterns for understanding SASM interannual variability are discussed.",
        "doi": "10.1175/JCLI-D-14-00612.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2015-05",
        "series_number": "9",
        "volume": "28",
        "issue": "9",
        "pages": "3731-3750"
    },
    {
        "id": "authors:w3rhj-tk931",
        "collection": "authors",
        "collection_id": "w3rhj-tk931",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150430-130410543",
        "type": "article",
        "title": "Why Eddy Momentum Fluxes are Concentrated in the Upper Troposphere",
        "author": [
            {
                "family_name": "Ait-Chaalal",
                "given_name": "Farid",
                "clpid": "Ait-Chaalal-F"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The extratropical eddy momentum flux (EMF) is controlled by generation, propagation, and dissipation of large-scale eddies and is concentrated in Earth's upper troposphere. An idealized GCM is used to investigate how this EMF structure arises. In simulations in which the poles are heated more strongly than the equator, EMF is concentrated near the surface, demonstrating that surface drag generally is not responsible for the upper-tropospheric EMF concentration. Although Earth's upper troposphere favors linear wave propagation, quasi-linear simulations in which nonlinear eddy\u2013eddy interactions are suppressed demonstrate that this is likewise not primarily responsible for the upper-tropospheric EMF concentration. The quasi-linear simulations reveal the essential role of nonlinear eddy\u2013eddy interactions in the surf zone in the upper troposphere, where wave activity absorption away from the baroclinic generation regions occurs through the nonlinear generation of small scales. In Earth-like atmospheres, wave activity that is generated in the lower troposphere propagates upward and then turns meridionally, eventually being absorbed nonlinearly in the upper troposphere. The level at which the wave activity begins to propagate meridionally appears to be set by the typical height reached by baroclinic eddies. This can coincide with the tropopause height but also can lie below it if convection controls the tropopause height. In the latter case, EMF is maximal well below the tropopause. The simulations suggest that EMF is concentrated in Earth's upper troposphere because typical baroclinic eddies reach the tropopause.",
        "doi": "10.1175/JAS-D-14-0243.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2015-04",
        "series_number": "4",
        "volume": "72",
        "issue": "4",
        "pages": "1585-1604"
    },
    {
        "id": "authors:s1hcf-xws73",
        "collection": "authors",
        "collection_id": "s1hcf-xws73",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20141222-085606925",
        "type": "article",
        "title": "Martian atmospheric collapse: Idealized GCM studies",
        "author": [
            {
                "family_name": "Soto",
                "given_name": "Alejandro",
                "clpid": "Soto-A"
            },
            {
                "family_name": "Mischna",
                "given_name": "Michael",
                "orcid": "0000-0002-8022-5319",
                "clpid": "Mischna-M-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Lee",
                "given_name": "Christopher",
                "clpid": "Lee-Christopher"
            },
            {
                "family_name": "Richardson",
                "given_name": "Mark",
                "clpid": "Richardson-M"
            }
        ],
        "abstract": "Global energy balance models of the Martian atmosphere predict that, for a range of total CO_2 inventories, the CO_2 atmosphere may condense until a state with a permanent polar cap is reached. This process, which is commonly referred to as atmospheric collapse, may limit the time available for physical and chemical weathering. The global energy balance models that predict atmospheric collapse represent the climate using simplified parameterizations for atmospheric processes such as radiative transfer and atmospheric heat transport. However, a more detailed representation of these atmospheric processes is critical when the atmosphere is near a transition, such as the threshold for collapse. Therefore, we use the Mars Weather Research and Forecasting (MarsWRF) general circulation model (GCM) to investigate how the explicit representation of meridional heat transport and more detailed radiative transfer affects the onset of atmospheric collapse. Using MarsWRF, we find that previous energy balance modeling underestimates the range of CO_2 inventories for which the atmosphere collapses and that the obliquity of Mars determines the range of CO_2 inventories that can collapse. For a much larger range of CO_2 inventories than expected, atmospheric heat transport is insufficient to prevent the atmospheric collapse. We show that the condensation of CO_2 onto Olympus Mons and adjacent mountains generates a condensation flow. This condensation flow syphons energy that would otherwise be transported poleward, which helps explain the large range of CO_2 inventories for which the atmosphere collapses.",
        "doi": "10.1016/j.icarus.2014.11.028",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2015-04",
        "volume": "250",
        "pages": "553-569"
    },
    {
        "id": "authors:herjn-ev120",
        "collection": "authors",
        "collection_id": "herjn-ev120",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150409-152635552",
        "type": "article",
        "title": "Physics of Changes in Synoptic Midlatitude Temperature Variability",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "P\u0142otka",
                "given_name": "Hanna",
                "clpid": "P\u0142otka-Hanna"
            }
        ],
        "abstract": "This paper examines the physical processes controlling how synoptic midlatitude temperature variability near the surface changes with climate. Because synoptic temperature variability is primarily generated by advection, it can be related to mean potential temperature gradients and mixing lengths near the surface. Scaling arguments show that the reduction of meridional potential temperature gradients that accompanies polar amplification of global warming leads to a reduction of the synoptic temperature variance near the surface. This is confirmed in simulations of a wide range of climates with an idealized GCM. In comprehensive climate simulations (CMIP5), Arctic amplification of global warming similarly entails a large-scale reduction of the near-surface temperature variance in Northern Hemisphere midlatitudes, especially in winter. The probability density functions of synoptic near-surface temperature variations in midlatitudes are statistically indistinguishable from Gaussian, both in reanalysis data and in a range of climates simulated with idealized and comprehensive GCMs. This indicates that changes in mean values and variances suffice to account for changes even in extreme synoptic temperature variations. Taken together, the results indicate that Arctic amplification of global warming leads to even less frequent cold outbreaks in Northern Hemisphere winter than a shift toward a warmer mean climate implies by itself.",
        "doi": "10.1175/JCLI-D-14-00632.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2015-03",
        "series_number": "6",
        "volume": "28",
        "issue": "6",
        "pages": "2312-2331"
    },
    {
        "id": "authors:8jewe-3nj46",
        "collection": "authors",
        "collection_id": "8jewe-3nj46",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150212-130610956",
        "type": "article",
        "title": "Scaling of Off-Equatorial Jets in Giant Planet Atmospheres",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "In the off-equatorial region of Jupiter's and Saturn's atmospheres, baroclinic eddies transport angular momentum out of retrograde and into prograde jets. In a statistically steady state, this angular momentum transfer by eddies must be balanced by dissipation, likely produced by magnetohydrodynamic (MHD) drag in the planetary interior. This paper examines systematically how an idealized representation of this drag in a general circulation model (GCM) of the upper atmosphere of giant planets modifies jet characteristics, the angular momentum budget, and the energy budget.\n\nIn the GCM, Rayleigh drag at an artificial lower boundary (with mean pressure of 3 bar) is used as a simple representation of the MHD drag that the flow on giant planets experiences at depth. As the drag coefficient decreases, the eddy length scale and eddy kinetic energy increase, as they do in studies of two-dimensional turbulence. Off-equatorial jets become wider and stronger, with increased interjet spacing. Coherent vortices also become more prevalent. Generally, the jet width scales with the Rhines scale, which is of similar magnitude as the Rossby radius in the simulations. The jet strength increases primarily through strengthening of the barotropic component, which increases as the drag coefficient decreases because the overall kinetic energy dissipation remains roughly constant. The overall kinetic energy dissipation remains roughly constant presumably because it is controlled by baroclinic conversion of potential to kinetic energy in the upper troposphere, which is mainly determined by the differential solar radiation and is only weakly dependent on bottom drag and barotropic flow variations.\n\nFor Jupiter and Saturn, these results suggest that the wider and stronger jets on Saturn may arise because the MHD drag on Saturn is weaker than on Jupiter, while the thermodynamic efficiencies of the atmospheres are not sensitive to the drag parameters.",
        "doi": "10.1175/JAS-D-13-0391.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2015-01",
        "series_number": "1",
        "volume": "72",
        "issue": "1",
        "pages": "389-408"
    },
    {
        "id": "authors:eqfnw-8k073",
        "collection": "authors",
        "collection_id": "eqfnw-8k073",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20141110-141049554",
        "type": "article",
        "title": "Role of Changes in Mean Temperatures versus Temperature Gradients in the Recent Widening of the Hadley Circulation",
        "author": [
            {
                "family_name": "Adam",
                "given_name": "Ori",
                "orcid": "0000-0003-0334-0636",
                "clpid": "Adam-Ori"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Harnik",
                "given_name": "Nili",
                "clpid": "Harnik-Nili"
            }
        ],
        "abstract": "The Hadley circulation (HC) has widened in recent decades, and it widens as the climate warms in simulations. But the mechanisms responsible for the widening remain unclear, and the widening in simulations is generally smaller than observed.\nTo identify mechanisms responsible for the HC widening and for model\u2013observation discrepancies, this study analyzes how interannual variations of tropical-mean temperatures and meridional temperature gradients influence the HC width. Changes in mean temperatures are part of any global warming signal, whereas changes in temperature gradients are primarily associated with ENSO. Within this study, 6 reanalysis datasets, 22 Atmospheric Modeling Intercomparison Project (AMIP) simulations, and 11 historical simulations from phase 5 of the Climate Modeling Intercomparison Project (CMIP5) are analyzed, covering the years 1979\u20132012. It is found that the HC widens as mean temperatures increase or as temperature gradients weaken in most reanalyses and climate models. On average, climate models exhibit a smaller sensitivity of HC width to changes in mean temperatures and temperature gradients than do reanalyses. However, the sensitivities differ substantially among reanalyses, rendering the HC response to mean temperatures in climate models not statistically different from that in reanalyses.\nWhile global-mean temperatures did not increase substantially between 1997 and 2012, the HC continued to widen in most reanalyses. The analysis here suggests that the HC widening from 1979 to 1997 is primarily the result of global warming, whereas the widening of the HC from 1997 to 2012 is associated with increased midlatitude temperatures and hence reduced temperature gradients during this period.",
        "doi": "10.1175/JCLI-D-14-00140.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2014-10",
        "series_number": "19",
        "volume": "27",
        "issue": "19",
        "pages": "7450-7461"
    },
    {
        "id": "authors:w9vtr-ma122",
        "collection": "authors",
        "collection_id": "w9vtr-ma122",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140908-094122453",
        "type": "article",
        "title": "Migrations and dynamics of the intertropical convergence zone",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Haug",
                "given_name": "Gerald H.",
                "clpid": "Haug-G-H"
            }
        ],
        "abstract": "Rainfall on Earth is most intense in the intertropical convergence zone (ITCZ), a narrow belt of clouds centred on average around six degrees north of the Equator. The mean position of the ITCZ north of the Equator arises primarily because the Atlantic Ocean transports energy northward across the Equator, rendering the Northern Hemisphere warmer than the Southern Hemisphere. On seasonal and longer timescales, the ITCZ migrates, typically towards a warming hemisphere but with exceptions, such as during El Ni\u00f1o events. An emerging framework links the ITCZ to the atmospheric energy balance and may account for ITCZ variations on timescales from years to geological epochs.",
        "doi": "10.1038/nature13636",
        "issn": "0028-0836",
        "publisher": "Nature Publishing Group",
        "publication": "Nature",
        "publication_date": "2014-09-04",
        "series_number": "7516",
        "volume": "513",
        "issue": "7516",
        "pages": "45-53"
    },
    {
        "id": "authors:hbexr-nz549",
        "collection": "authors",
        "collection_id": "hbexr-nz549",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140829-083755173",
        "type": "article",
        "title": "Constraining the depth of Saturn's zonal winds by measuring thermal and gravitational signals",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Fletcher",
                "given_name": "Leigh N.",
                "orcid": "0000-0001-5834-9588",
                "clpid": "Fletcher-L-N"
            }
        ],
        "abstract": "Based on straightforward dynamical considerations, we show how available and upcoming measurements of Saturn's thermal and gravitational signals can be used to constrain the depth to which its zonal winds penetrate. The dynamical considerations issue from the facts that Saturn has a strong intrinsic heat flux, rotates rapidly, and has negligible atmospheric viscosity. As a result, convective motions align with surfaces of constant specific angular momentum, which are, away from the equator, approximately cylinders concentric with the planet's spin axis. Convective motions in the interior therefore tend to homogenize entropy in the direction of the spin axis, but not necessarily perpendicular to it. Using the assumption of interior entropy homogenization in the direction of the spin axis, we determine the zonal winds and their associated thermal and gravitational signals by combining thermal wind balance, the equation of state, the observed zonal winds at the cloud level, and estimates of the strength of the magnetohydrodynamic (MHD) drag that zonal winds experience in the deep interior.\n\nWe find zonal winds likely extend deeply into Saturn, to a depth between about 0.630.63 and 0.83R_S(with Saturn's radius R_S), or to pressures between 1.4 and 0.3 Mbar. The equation of state of hydrogen constrains zonal winds with strengths similar to the cloud level winds to be confined within the outer few percent of Saturn's radius, with substantially weaker winds below, irrespective of where in the range of plausible estimates Saturn's imprecisely known rotation rate falls. Depending on the rotation rate and the precise depth to which zonal winds penetrate, we estimate that the meridional equator-to-pole temperature contrasts in thermal wind balance with the inferred zonal winds increase with depth and reach 1\u20132 K at 1 bar and 2\u20134 K at 5 bar. They would be much larger if the cutoff radii of the zonal winds were much shallower than we estimate, but thermal observations by the Cassini Composite Infrared Spectrometer (CIRS) already rule out very shallow flows: Zonal winds must extend deeper than 5000 bar (0.965R_S) because otherwise the associated equator-to-pole contrast would be inconsistent with Cassini CIRS retrievals of the temperature field.\n\nUpcoming Cassini gravitational measurements can further constrain the penetration depth of zonal winds, as gravitational zonal harmonics associated with deep zonal winds are much larger than those associated with shallow zonal winds. The even gravitational zonal harmonics associated with zonal winds that penetrate to megabar levels start to become distinguishable from the planetary solid body rotation at zonal harmonic degree n\u22738n\u22738. The low-order odd gravitational zonal harmonics, which do not depend on the planetary solid body rotation, will be detectable within likely Cassini measurement errors for cutoff radii r_c\u22720.98R_S (\u22731000 bar). Combining thermal and gravitational signals of the zonal winds, the penetration depths of the zonal winds relative to different rotation rates can thus be constrained.",
        "doi": "10.1016/j.icarus.2014.05.036",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2014-09-01",
        "volume": "239",
        "pages": "260-272"
    },
    {
        "id": "authors:tme1k-y4547",
        "collection": "authors",
        "collection_id": "tme1k-y4547",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140728-091222072",
        "type": "article",
        "title": "Energetic Constraints on the Position of the Intertropical Convergence Zone",
        "author": [
            {
                "family_name": "Bischoff",
                "given_name": "Tobias",
                "orcid": "0000-0003-3930-2762",
                "clpid": "Bischoff-Tobias"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The intertropical convergence zone (ITCZ) can shift meridionally on seasonal and longer time scales. Previous studies have shown that the latitude of the ITCZ is negatively correlated with cross-equatorial atmospheric energy transport. For example, the ITCZ shifts southward as the Northern Hemisphere cools and the northward cross-equatorial energy transport strengthens in response. It has remained unclear what controls the sensitivity of the ITCZ position to cross-equatorial energy transport and what other factors may lead to shifts of the ITCZ position. Here it is shown that the sensitivity of the ITCZ position to cross-equatorial energy transport depends on the net energy input to the equatorial atmosphere: the net radiative energy input minus any energy uptake by the oceans. Changes in this energy input can also lead to ITCZ shifts. The cross-equatorial energy transport is related through a series of approximations to interhemispheric asymmetries in the near-surface temperature distribution. The resulting theory of the ITCZ position is tested in idealized general circulation model simulations with a slab ocean as lower boundary condition. In the simulations, cross-equatorial energy transport increases under global warming (primarily because extratropical latent energy fluxes strengthen), and this shifts the ITCZ poleward. The ITCZ shifts equatorward if primarily the tropics warm in response to an increased net energy input to the equatorial atmosphere. The results have implications for explaining the varied response of the ITCZ to global or primarily tropical changes in the atmospheric energy balance, such as those that occur under global warming or El Ni\u00f1o.",
        "doi": "10.1175/JCLI-D-13-00650.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2014-07",
        "series_number": "13",
        "volume": "27",
        "issue": "13",
        "pages": "4937-4951"
    },
    {
        "id": "authors:zfy9g-brx31",
        "collection": "authors",
        "collection_id": "zfy9g-brx31",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140106-112443566",
        "type": "article",
        "title": "Storm Track Shifts under Climate Change: What Can Be Learned from Large-Scale Dry Dynamics",
        "author": [
            {
                "family_name": "Mbengue",
                "given_name": "Cheikh",
                "clpid": "Mbengue-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Earth's storm tracks are instrumental for transporting heat, momentum, and moisture and thus strongly influence the surface climate. Climate models, supported by a growing body of observational data, have demonstrated that storm tracks shift poleward as the climate warms. But the dynamical mechanisms responsible for this shift remain unclear. To isolate what portion of the storm track shift may be accounted for by large-scale dry dynamics alone, disregarding the latent heat released in phase changes of water, this study investigates the storm track shift under various kinds of climate change in an idealized dry general circulation model (GCM) with an adjustable but constant convective stability. It is found that increasing the mean surface temperature or the convective stability leads to poleward shifts of storm tracks, even if the convective stability is increased only in a narrow band around the equator. Under warming and convective stability changes roughly corresponding to a doubling of CO_2 concentrations from a present-day Earthlike climate, storm tracks shift about 0.8\u00b0 poleward, somewhat less than but in qualitative agreement with studies using moist GCMs. About 63% (0.5\u00b0) of the poleward shift is shown to be caused by tropical convective stability variations. This demonstrates that tropical processes alone (the increased dry static stability of a warmer moist adiabat) can account for part of the poleward shift of storm tracks under global warming. This poleward shift generally occurs in tandem with a poleward expansion of the Hadley circulation; however, the Hadley circulation expansion does not always parallel the storm track shift.",
        "doi": "10.1175/JCLI-D-13-00404.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2013-12",
        "series_number": "24",
        "volume": "26",
        "issue": "24",
        "pages": "9923-9930"
    },
    {
        "id": "authors:tf4xm-0g263",
        "collection": "authors",
        "collection_id": "tf4xm-0g263",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130903-102819440",
        "type": "article",
        "title": "The Role of Stationary Eddies in Shaping Midlatitude Storm Tracks",
        "author": [
            {
                "family_name": "Kaspi",
                "given_name": "Yohai",
                "orcid": "0000-0003-4089-0020",
                "clpid": "Kaspi-Y"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Transient and stationary eddies shape the extratropical climate through their transport of heat, moisture, and momentum. In the zonal mean, the transports by transient eddies dominate over those by stationary eddies, but this is not necessarily the case locally. In particular, in storm-track entrance and exit regions during winter, stationary eddies and their interactions with the mean flow dominate the atmospheric energy transport. Here it is shown that stationary eddies can shape storm tracks and control where they terminate by modifying local baroclinicity. Simulations with an idealized aquaplanet GCM show that zonally localized surface heating alone (e.g., ocean heat flux convergence) gives rise to storm tracks, which have a well-defined length scale that is similar to that of Earth's storm tracks. The storm tracks terminate downstream of the surface heating even in the absence of continents, at a distance controlled by the stationary Rossby wavelength scale. Stationary eddies play a dual role: within about half a Rossby wavelength downstream of the heating region, stationary eddy energy fluxes increase the baroclinicity and therefore contribute to energizing the storm track; farther downstream, enhanced poleward and upward energy transport by stationary eddies reduces the baroclinicity by reducing the meridional temperature gradients and enhancing the static stability. Transports both of sensible and latent heat (water vapor) play important roles in determining where storm tracks terminate.",
        "doi": "10.1175/JAS-D-12-082.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2013-08",
        "series_number": "8",
        "volume": "70",
        "issue": "8",
        "pages": "2596-2613"
    },
    {
        "id": "authors:9bk4e-hb562",
        "collection": "authors",
        "collection_id": "9bk4e-hb562",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130813-150947854",
        "type": "article",
        "title": "Wind driven capillary-gravity waves on Titan's lakes: Hard to detect or non-existent?",
        "author": [
            {
                "family_name": "Hayes",
                "given_name": "A. G.",
                "clpid": "Hayes-A-G"
            },
            {
                "family_name": "Lorenz",
                "given_name": "R. D.",
                "orcid": "0000-0001-8528-4644",
                "clpid": "Lorenz-R-D"
            },
            {
                "family_name": "Donelan",
                "given_name": "M. A.",
                "clpid": "Donelan-M-A"
            },
            {
                "family_name": "Manga",
                "given_name": "M.",
                "clpid": "Manga-M"
            },
            {
                "family_name": "Lunine",
                "given_name": "J. I.",
                "orcid": "0000-0003-2279-4131",
                "clpid": "Lunine-Jonathan-Irving"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Lamb",
                "given_name": "M. P.",
                "orcid": "0000-0002-5701-0504",
                "clpid": "Lamb-M-P"
            },
            {
                "family_name": "Mitchell",
                "given_name": "J. M.",
                "clpid": "Mitchell-J-M"
            },
            {
                "family_name": "Fischer",
                "given_name": "W. W.",
                "orcid": "0000-0002-8836-3054",
                "clpid": "Fischer-W-W"
            },
            {
                "family_name": "Graves",
                "given_name": "S. D.",
                "clpid": "Graves-S-D"
            },
            {
                "family_name": "Tolman",
                "given_name": "H. L.",
                "clpid": "Tolman-H-L"
            },
            {
                "family_name": "Aharonson",
                "given_name": "O.",
                "orcid": "0000-0001-9930-2495",
                "clpid": "Aharonson-O"
            },
            {
                "family_name": "Encrenaz",
                "given_name": "P. J.",
                "clpid": "Encrenaz-P-J"
            },
            {
                "family_name": "Ventura",
                "given_name": "B.",
                "clpid": "Ventura-B"
            },
            {
                "family_name": "Casarano",
                "given_name": "D.",
                "clpid": "Casarano-D"
            },
            {
                "family_name": "Notarnicola",
                "given_name": "C.",
                "clpid": "Notarnicola-C"
            }
        ],
        "abstract": "Saturn's moon Titan has lakes and seas of liquid hydrocarbon and a dense atmosphere, an environment conducive to generating wind waves. Cassini observations thus far, however, show no indication of waves. We apply models for wind wave generation and detection to the Titan environment. Results suggest wind speed thresholds at a reference altitude of 10 m of 0.4\u20130.7 m/s for liquid compositions varying between pure methane and equilibrium mixtures with the atmosphere (ethane has a threshold of 0.6 m/s), varying primarily with liquid viscosity. This reduced threshold, as compared to Earth, results from Titan's increased atmosphere-to-liquid density ratio, reduced gravity and lower surface tension. General Circulation Models (GCMs) predict wind speeds below derived thresholds near equinox, when available observations of lake surfaces have been acquired. Predicted increases in winds as Titan approaches summer solstice, however, will exceed expected thresholds and may provide constraints on lake composition and/or GCM accuracy through the presence or absence of waves during the Cassini Solstice Mission. A two-scale microwave backscatter model suggests that returns from wave-modified liquid hydrocarbon surfaces may be below the pixel-scale noise floor of Cassini radar images, but can be detectable using real-aperture scatterometry, pixel binning and/or observations obtained in a specular geometry.",
        "doi": "10.1016/j.icarus.2013.04.004",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2013-07",
        "series_number": "1",
        "volume": "225",
        "issue": "1",
        "pages": "403-412"
    },
    {
        "id": "authors:0wjhh-rq195",
        "collection": "authors",
        "collection_id": "0wjhh-rq195",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130712-132448635",
        "type": "article",
        "title": "The Force Balance of the Southern Ocean Meridional Overturning Circulation",
        "author": [
            {
                "family_name": "Mazloff",
                "given_name": "Matthew R.",
                "clpid": "Mazloff-M-R"
            },
            {
                "family_name": "Ferrari",
                "given_name": "Raffaele",
                "orcid": "0000-0003-1895-4294",
                "clpid": "Ferrari-R"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The Southern Ocean (SO) limb of the meridional overturning circulation (MOC) is characterized by three vertically stacked cells, each with a transport of about 10 Sv (Sv \u2261 10^6 m^3 s^(\u22121)). The buoyancy transport in the SO is dominated by the upper and middle MOC cells, with the middle cell accounting for most of the buoyancy transport across the Antarctic Circumpolar Current. A Southern Ocean state estimate for the years 2005 and 2006 with 1/6\u00b0 resolution is used to determine the forces balancing this MOC. Diagnosing the zonal momentum budget in density space allows an exact determination of the adiabatic and diapycnal components balancing the thickness-weighted (residual) meridional transport. It is found that, to lowest order, the transport consists of an eddy component, a directly wind-driven component, and a component in balance with mean pressure gradients. Nonvanishing time-mean pressure gradients arise because isopycnal layers intersect topography or the surface in a circumpolar integral, leading to a largely geostrophic MOC even in the latitude band of Drake Passage. It is the geostrophic water mass transport in the surface layer where isopycnals outcrop that accomplishes the poleward buoyancy transport.",
        "doi": "10.1175/JPO-D-12-069.1",
        "issn": "0022-3670",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Physical Oceanography",
        "publication_date": "2013-06",
        "series_number": "6",
        "volume": "43",
        "issue": "6",
        "pages": "1193-1208"
    },
    {
        "id": "authors:0g7yc-t4q13",
        "collection": "authors",
        "collection_id": "0g7yc-t4q13",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130606-083406918",
        "type": "article",
        "title": "Predictions of thermal and gravitational signals of Jupiter's deep zonal winds",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Kaspi",
                "given_name": "Yohai",
                "orcid": "0000-0003-4089-0020",
                "clpid": "Kaspi-Y"
            }
        ],
        "abstract": "NASA's Juno spacecraft will make microwave and gravity measurements of Jupiter. These can reveal information about the composition of Jupiter's atmosphere and about the temperature and density structure below the visible clouds, which is in balance with the structure of the zonal winds. Here we show that there exist strong physical constraints on the structure of the off-equatorial deep zonal winds, and that these imply dynamical constraints on the thermal and gravitational signals Juno will measure. The constraints derive from the facts that Jupiter is rapidly rotating, has nearly inviscid flow, and has strong intrinsic heat fluxes emanating from the deep interior. Because of the strong intrinsic heat fluxes, Jupiter's interior is convecting, but the rapid rotation and weak viscosity constrain the convective motions away from the equator to occur primarily along cylinders parallel to the planet's spin axis. As a consequence, convection is expected to approximately homogenize entropy along the spin axis, thereby adjusting the interior to a convectively and inertially nearly neutral state. In this state, entropy gradients perpendicular to the spin axis are constant but generally not zero on cylinders concentric with the spin axis. Additionally, thermal wind balance relates entropy gradients perpendicular to the spin axis to the zonal wind shear between the observed cloud-level winds and winds in the deep interior (pressures of order 10^6 bar), which must be much weaker because otherwise the Ohmic energy dissipation produced by the interaction of the zonal winds with the planetary magnetic field would exceed the planetary luminosity. Combining these physical constraints with thermal and electrical properties of the atmosphere, we obtain that zonal winds away from the equator likely extend deeply into Jupiter (to a depth between about 0.84R_J and 0.94R_J with Jupiter radius R_J) but have strengths similar to cloud level winds only within the outer few percent of Jupiter's radius. Meridional equator-to-pole temperature contrasts in thermal wind balance with the zonal winds increase with depth and reach \u223c1\u20132 K at 50 bar; they would reach O(10 K) if the winds were shallowly confined, as has been proposed previously. Such temperature contrasts will be detectable by Juno's microwave instrument and are expected to be much larger than those associated with variations in water vapor abundance. The associated gravitational signals of the zonal winds will also be detectable by Juno, but they will be more difficult to distinguish from those implied by other flow models with deep zonal flows. The combination of Juno's gravity and microwave instruments should be able to distinguish deep flows (detectable gravitational signals) from shallow flows (detectable thermal signals), providing strong constraints on the penetration depth of substantial zonal winds.",
        "doi": "10.1016/j.icarus.2013.01.025",
        "issn": "0019-1035",
        "publisher": "Elsevier",
        "publication": "Icarus",
        "publication_date": "2013-05",
        "series_number": "1",
        "volume": "224",
        "issue": "1",
        "pages": "114-125"
    },
    {
        "id": "authors:n9vaf-mr677",
        "collection": "authors",
        "collection_id": "n9vaf-mr677",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130425-090941220",
        "type": "article",
        "title": "The Tropical Precipitation Response to Orbital Precession",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "clpid": "Eisenman-I"
            }
        ],
        "abstract": "Orbital precession changes the seasonal distribution of insolation at a given latitude but not the annual mean. Hence, the correlation of paleoclimate proxies of annual-mean precipitation with orbital precession implies a nonlinear rectification in the precipitation response to seasonal solar forcing. It has previously been suggested that the relevant nonlinearity is that of the Clausius\u2013Clapeyron relationship. Here it is argued that a different nonlinearity related to moisture advection by the atmospheric circulation is more important. When perihelion changes from one hemisphere's summer solstice to the other's in an idealized aquaplanet atmospheric general circulation model, annual-mean precipitation increases in the hemisphere with the brighter, warmer summer and decreases in the other hemisphere, in qualitative agreement with paleoclimate proxies that indicate such hemispherically antisymmetric climate variations. The rectification mechanism that gives rise to the precipitation changes is identified by decomposing the perturbation water vapor budget into \"thermodynamic\" and \"dynamic\" components. Thermodynamic changes (caused by changes in humidity with unchanged winds) dominate the hemispherically antisymmetric annual-mean precipitation response to precession in the absence of land\u2013sea contrasts. The nonlinearity that enables the thermodynamic changes to affect annual-mean precipitation is a nonlinearity of moisture advection that arises because precession-induced seasonal humidity changes correlate with the seasonal cycle in low-level convergence. This interpretation is confirmed using simulations in which the Clausius\u2013Clapeyron relationship is explicitly linearized. The thermodynamic mechanism also operates in simulations with an idealized representation of land, although in these simulations the dynamic component of the precipitation changes is also important, adding to the thermodynamic precipitation changes in some latitudes and offsetting it in others.",
        "doi": "10.1175/JCLI-D-12-00186.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2013-03",
        "series_number": "6",
        "volume": "26",
        "issue": "6",
        "pages": "2010-2021"
    },
    {
        "id": "authors:91g54-kbx80",
        "collection": "authors",
        "collection_id": "91g54-kbx80",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130308-075759181",
        "type": "article",
        "title": "Hadley Circulation Response to Orbital Precession. Part I: Aquaplanets",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "clpid": "Eisenman-I"
            }
        ],
        "abstract": "The response of the monsoonal and annual-mean Hadley circulation to orbital precession is examined in an idealized atmospheric general circulation model with an aquaplanet slab-ocean lower boundary. Contrary to expectations, the simulated monsoonal Hadley circulation is weaker when perihelion occurs at the summer solstice than when aphelion occurs at the summer solstice. The angular momentum balance and energy balance are examined to understand the mechanisms that produce this result. That the summer with stronger insolation has a weaker circulation is the result of an increase in the atmosphere's energetic stratification, the gross moist stability, which increases more than the amount required to balance the change in atmospheric energy flux divergence necessitated by the change in top-of-atmosphere net radiation. The solstice-season changes result in annual-mean Hadley circulation changes (e.g., changes in circulation strength).",
        "doi": "10.1175/JCLI-D-11-00716.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2013-02-01",
        "series_number": "3",
        "volume": "26",
        "issue": "3",
        "pages": "740-753"
    },
    {
        "id": "authors:m3h3x-e9t29",
        "collection": "authors",
        "collection_id": "m3h3x-e9t29",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130307-111836691",
        "type": "article",
        "title": "Hadley Circulation Response to Orbital Precession. Part II: Subtropical Continent",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "clpid": "Eisenman-I"
            }
        ],
        "abstract": "The response of the monsoonal and annual-mean Hadley circulation to orbital precession is examined in an idealized atmospheric general circulation model with a simplified representation of land surface processes in subtropical latitudes. When perihelion occurs in the summer of a hemisphere with a subtropical continent, changes in the top-of-atmosphere energy balance, together with a poleward shift of the monsoonal circulation boundary, lead to a strengthening of the monsoonal circulation. Spatial variations in surface heat capacity determine whether radiative perturbations are balanced by energy storage or by atmospheric energy fluxes. Although orbital precession does not affect annual-mean insolation, the annual-mean Hadley circulation does respond to orbital precession because its sensitivity to radiative changes varies over the course of the year: the monsoonal circulation in summer is near the angular momentum-conserving limit and responds directly to radiative changes; whereas in winter, the circulation is affected by the momentum fluxes of extratropical eddies and is less sensitive to radiative changes.",
        "doi": "10.1175/JCLI-D-12-00149.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2013-02",
        "series_number": "3",
        "volume": "26",
        "issue": "3",
        "pages": "754-771"
    },
    {
        "id": "authors:rdd74-w7771",
        "collection": "authors",
        "collection_id": "rdd74-w7771",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20130806-093803561",
        "type": "article",
        "title": "Continental arc\u2013island arc fluctuations, growth of crustal carbonates, and long-term climate change",
        "author": [
            {
                "family_name": "Lee",
                "given_name": "Cin-Ty A.",
                "clpid": "Lee-Cin-Ty-A"
            },
            {
                "family_name": "Shen",
                "given_name": "Bing",
                "clpid": "Shen-Bing"
            },
            {
                "family_name": "Slotnick",
                "given_name": "Benjamin S.",
                "clpid": "Slotnick-B-S"
            },
            {
                "family_name": "Liao",
                "given_name": "Kelley",
                "clpid": "Liao-Kelley"
            },
            {
                "family_name": "Dickens",
                "given_name": "Gerald R.",
                "clpid": "Dickens-G-R"
            },
            {
                "family_name": "Yokoyama",
                "given_name": "Yusuke",
                "clpid": "Yokoyama-Yusuke"
            },
            {
                "family_name": "Lenardic",
                "given_name": "Adrian",
                "clpid": "Lenardic-A"
            },
            {
                "family_name": "Dasgupta",
                "given_name": "Rajdeep",
                "clpid": "Dasgupta-R"
            },
            {
                "family_name": "Jellinek",
                "given_name": "Mark",
                "clpid": "Jellinek-M"
            },
            {
                "family_name": "Lackey",
                "given_name": "Jade Star",
                "clpid": "Lackey-J-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Tice",
                "given_name": "Michael M.",
                "clpid": "Tice-M-M"
            }
        ],
        "abstract": "The Cretaceous to early Paleogene (ca. 140\u201350 Ma) was characterized by a greenhouse baseline climate, driven by elevated concentrations of atmospheric CO_2. Hypotheses for the elevated CO_2 concentrations invoke an increase in volcanic CO_2 production due to higher oceanic crust production rates, higher frequency of large igneous provinces, or increases in pelagic carbonate deposition, the last leading to enhanced carbonate subduction into the mantle source regions of arc volcanoes. However, these are not the only volcanic sources of CO_2 during this time interval. We show here that ocean-continent subduction zones, manifested as a global chain of continental arc volcanoes, were as much as 200% longer in the Cretaceous and early Paleogene than in the late Paleogene to present, when a cooler climate prevailed. In particular, many of these continental arcs, unlike island arcs, intersected ancient continental platform carbonates stored on the continental upper plate. We show that the greater length of Cretaceous\u2013Paleogene continental arcs, specifically carbonate-intersecting arcs, could have increased global production of CO_2 by at least 3.7\u20135.5 times that of the present day. This magmatically driven crustal decarbonation flux of CO_2 through continental arcs exceeds that delivered by Cretaceous oceanic crust production, and was sufficient to drive Cretaceous\u2013Paleogene greenhouse conditions. Thus, carbonate-intersecting continental arc volcanoes likely played an important role in driving greenhouse conditions in the Cretaceous\u2013Paleogene. If so, the waning of North American and Eurasian continental arcs in the Late Cretaceous to early Paleogene, followed by a fundamental shift in western Pacific subduction zones ca. 52 Ma to an island arc\u2013dominated regime, would have been manifested as a decline in global volcanic CO_2 production, prompting a return to an icehouse baseline in the Neogene. Our analysis leads us to speculate that long-term (&gt;50 m.y.) greenhouse-icehouse oscillations may be linked to fluctuations between continental- and island arc\u2013dominated states. These tectonic fluctuations may result from large-scale changes in the nature of subduction zones, changes we speculate may be tied to the assembly and dispersal of continents. Specifically, dispersal of continents may drive the leading edge of continents to override subduction zones, resulting in continental arc volcanism, whereas assembly of continents or closing of large ocean basins may be manifested as large-scale slab rollback, resulting in the development of intraoceanic volcanic arcs. We suggest that greenhouse-icehouse oscillations are a natural consequence of plate tectonics operating in the presence of continental masses, serving as a large capacitor of carbonates that can be episodically purged during global flare-ups in continental arcs. Importantly, if the global crustal carbonate reservoir has grown with time, as might be expected because platform carbonates on continents do not generally subduct, the greenhouse-driving potential of continental arcs would have been small during the Archean, but would have increased in the Neoproterozoic and Phanerozoic after a significant reservoir of crustal carbonates had formed in response to the evolution of life and the growth of continents.",
        "doi": "10.1130/GES00822.1",
        "issn": "1553-040X",
        "publisher": "Geological Society of America",
        "publication": "Geosphere",
        "publication_date": "2013-02",
        "series_number": "1",
        "volume": "9",
        "issue": "1",
        "pages": "21-36"
    },
    {
        "id": "authors:fck90-56g57",
        "collection": "authors",
        "collection_id": "fck90-56g57",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20140717-110834015",
        "type": "article",
        "title": "The imprint of surface fluxes and transport on variations in total column carbon dioxide",
        "author": [
            {
                "family_name": "Keppel-Aleks",
                "given_name": "G.",
                "clpid": "Keppel-Aleks-G"
            },
            {
                "family_name": "Wennberg",
                "given_name": "P. O.",
                "orcid": "0000-0002-6126-3854",
                "clpid": "Wennberg-P-O"
            },
            {
                "family_name": "Washenfelder",
                "given_name": "R. A.",
                "orcid": "0000-0002-8106-3702",
                "clpid": "Washenfelder-R-A"
            },
            {
                "family_name": "Wunch",
                "given_name": "D.",
                "orcid": "0000-0002-4924-0377",
                "clpid": "Wunch-D"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Toon",
                "given_name": "G. C.",
                "orcid": "0000-0003-4174-7541",
                "clpid": "Toon-G-C"
            },
            {
                "family_name": "Andres",
                "given_name": "R. J.",
                "clpid": "Andres-R-J"
            },
            {
                "family_name": "Blavier",
                "given_name": "J. F.",
                "clpid": "Blavier-J-F-L"
            },
            {
                "family_name": "Connor",
                "given_name": "B.",
                "clpid": "Connor-B"
            },
            {
                "family_name": "Davis",
                "given_name": "K. J.",
                "clpid": "Davis-K-J"
            },
            {
                "family_name": "Desai",
                "given_name": "A. R.",
                "clpid": "Desai-A-R"
            },
            {
                "family_name": "Messerschmidt",
                "given_name": "J.",
                "clpid": "Messerschmidt-J"
            },
            {
                "family_name": "Notholt",
                "given_name": "J.",
                "clpid": "Notholt-J"
            },
            {
                "family_name": "Roehl",
                "given_name": "C. M.",
                "orcid": "0000-0001-5383-8462",
                "clpid": "Roehl-C-M"
            },
            {
                "family_name": "Sherlock",
                "given_name": "V.",
                "clpid": "Sherlock-V"
            },
            {
                "family_name": "Stephens",
                "given_name": "B. B.",
                "clpid": "Stephens-B-B"
            },
            {
                "family_name": "Vay",
                "given_name": "S. A.",
                "clpid": "Vay-S-A"
            },
            {
                "family_name": "Wofsy",
                "given_name": "S. C.",
                "orcid": "0000-0002-3990-6737",
                "clpid": "Wofsy-S-C"
            }
        ],
        "abstract": "New observations of the vertically integrated CO_2 mixing ratio, \u27e8CO_2\u27e9, from ground-based remote sensing show that variations in CO_2\u27e9 are primarily determined by large-scale flux patterns. They therefore provide fundamentally different information than observations made within the boundary layer, which reflect the combined influence of large-scale and local fluxes. Observations of both \u27e8CO_2\u27e9 and CO_2 concentrations in the free troposphere show that large-scale spatial gradients induce synoptic-scale temporal variations in \u27e8CO_2\u27e9 in the Northern Hemisphere midlatitudes through horizontal advection. Rather than obscure the signature of surface fluxes on atmospheric CO_2, these synoptic-scale variations provide useful information that can be used to reveal the meridional flux distribution. We estimate the meridional gradient in \u27e8CO_2\u27e9 from covariations in \u27e8CO_2\u27e9 and potential temperature, \u03b8, a dynamical tracer, on synoptic timescales to evaluate surface flux estimates commonly used in carbon cycle models. We find that simulations using Carnegie Ames Stanford Approach (CASA) biospheric fluxes underestimate both the \u27e8CO_2\u27e9 seasonal cycle amplitude throughout the Northern Hemisphere midlatitudes and the meridional gradient during the growing season. Simulations using CASA net ecosystem exchange (NEE) with increased and phase-shifted boreal fluxes better fit the observations. Our simulations suggest that climatological mean CASA fluxes underestimate boreal growing season NEE (between 45\u201365\u00b0 N) by ~40%. We describe the implications for this large seasonal exchange on inference of the net Northern Hemisphere terrestrial carbon sink.",
        "doi": "10.5194/bg-9-875-2012",
        "issn": "1726-4170",
        "publisher": "European Geosciences Union",
        "publication": "Biogeosciences",
        "publication_date": "2012-03-01",
        "series_number": "3",
        "volume": "9",
        "issue": "3",
        "pages": "875-891"
    },
    {
        "id": "authors:zyc6n-b1087",
        "collection": "authors",
        "collection_id": "zyc6n-b1087",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120807-101117478",
        "type": "article",
        "title": "Recovery and characterization of Neptune's near-polar stratospheric hot spot",
        "author": [
            {
                "family_name": "Orton",
                "given_name": "Glenn S.",
                "orcid": "0000-0001-7871-2823",
                "clpid": "Orton-G-S"
            },
            {
                "family_name": "Fletcher",
                "given_name": "Leigh N.",
                "orcid": "0000-0001-5834-9588",
                "clpid": "Fletcher-L-N"
            },
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Yanamandra-Fisher",
                "given_name": "Padma A.",
                "clpid": "Yanamandra-Fisher-P-A"
            },
            {
                "family_name": "de Pater",
                "given_name": "Imke",
                "orcid": "0000-0002-4278-3168",
                "clpid": "de-Pater-I"
            },
            {
                "family_name": "Edwards",
                "given_name": "Michelle",
                "clpid": "Edwards-M"
            },
            {
                "family_name": "Geballe",
                "given_name": "Thomas R.",
                "clpid": "Geballe-T-R"
            },
            {
                "family_name": "Hammel",
                "given_name": "Heidi B.",
                "orcid": "0000-0001-8751-3463",
                "clpid": "Hammel-H-B"
            },
            {
                "family_name": "Fujiyoshi",
                "given_name": "Takuya",
                "clpid": "Fujiyoshi-Takuya"
            },
            {
                "family_name": "Encrenaz",
                "given_name": "Therese",
                "clpid": "Encrenaz-T"
            },
            {
                "family_name": "Pantin",
                "given_name": "Eric",
                "clpid": "Pantin-E"
            },
            {
                "family_name": "Mousis",
                "given_name": "Olivier",
                "clpid": "Mousis-O"
            },
            {
                "family_name": "Fuse",
                "given_name": "Tetsuharu",
                "clpid": "Fuse-Tetsuharu"
            }
        ],
        "abstract": "Images of Neptune obtained in 2006 at ESO's Very Large Telescope (Orton et al., 2007, Astronomy &amp; Astrophysics 473, L5) revealed a near-polar hot spot near 70\u00b0S latitude that was detectable in filters sampling both stratospheric methane (7 \u03bcm) and ethane (\u223c12 \u03bcm) emission. Such a feature was not present in 2003 Keck and 2005 Gemini North observations, which showed only a general warming trend toward Neptune's pole that was longitudinally homogeneous. Because of the paucity of longitudinal sampling in the 2003, 2005 and 2006 images, it was not clear whether the failure to see this phenomenon in 2003 and 2005 was simply the result of insufficient longitudinal sampling or whether the phenomenon was truly variable in time. To unravel these two possibilities, we made follow-up observations on large telescopes that were capable of resolving Neptune at thermal-infrared wavelengths: Gemini South in 2007 and 2010 using the T-ReCS instrument, Subaru in 2008 using the COMICS instrument and VLT in 2008 and 2009 using the VISIR instrument. Two serendipitous T-ReCS images of Neptune were also obtained in 2007 using a broad N-band (8\u201314 \u03bcm) filter, whose radiance is dominated by stratospheric emission from both methane and ethane. The feature was recovered (i) in 2007 with T-ReCS in the broad N-band image and (ii) in 2008 with COMICS in a 12.5-\u03bcm image. However, T-ReCS observations in 2010 that covered up to 250\u00b0 of longitude did not show evidence of an off-polar hot spot. Although we have not definitively ruled out the possibility that various observers have simply missed a semi-permanent feature, it seems statistically very unlikely to be the case. With only 3 sightings in 13 independent observing epochs, it is likely that the phenomenon is ephemeral in time. A possible origin for the phenomenon is a large planetary wave that is dynamically confined to the high-latitude regions characterized by prograde zonal winds. It may be episodically excited by dynamical activity deeper in the atmosphere. This must be coupled with mixing near the poles that destroys or at least substantially attenuates the hot spot over the south pole that leads to an appearance of the typical polar stratospheric hot spot being offset in latitude.",
        "doi": "10.1016/j.pss.2011.06.013",
        "issn": "0032-0633",
        "publisher": "Elsevier",
        "publication": "Planetary and Space Science",
        "publication_date": "2012-02",
        "series_number": "1",
        "volume": "61",
        "issue": "1",
        "pages": "161-167"
    },
    {
        "id": "authors:g6pa1-5ff71",
        "collection": "authors",
        "collection_id": "g6pa1-5ff71",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120113-130450759",
        "type": "article",
        "title": "Polar methane accumulation and rainstorms on Titan from simulations of the methane cycle",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Graves",
                "given_name": "S. D. B.",
                "clpid": "Graves-S-D-B"
            },
            {
                "family_name": "Schaller",
                "given_name": "E. L.",
                "clpid": "Schaller-E-L"
            },
            {
                "family_name": "Brown",
                "given_name": "M. E.",
                "orcid": "0000-0002-8255-0545",
                "clpid": "Brown-M-E"
            }
        ],
        "abstract": "Titan has a methane cycle akin to Earth's water cycle. It has lakes in polar regions, preferentially in the north; dry low latitudes with fluvial features and occasional rainstorms; and tropospheric clouds mainly (so far) in southern middle latitudes and polar regions. Previous models have explained the low-latitude dryness as a result of atmospheric methane transport into middle and high latitudes. Hitherto, no model has explained why lakes are found only in polar regions and preferentially in the north; how low-latitude rainstorms arise; or why clouds cluster in southern middle and high latitudes. Here we report simulations with a three-dimensional atmospheric model coupled to a dynamic surface reservoir of methane. We find that methane is cold-trapped and accumulates in polar regions, preferentially in the north because the northern summer, at aphelion, is longer and has greater net precipitation than the southern summer. The net precipitation in polar regions is balanced in the annual mean by slow along-surface methane transport towards mid-latitudes, and subsequent evaporation. In low latitudes, rare but intense storms occur around the equinoxes, producing enough precipitation to carve surface features. Tropospheric clouds form primarily in middle and high latitudes of the summer hemisphere, which until recently has been the southern hemisphere. We predict that in the northern polar region, prominent clouds will form within about two (Earth) years and lake levels will rise over the next fifteen years.",
        "doi": "10.1038/nature10666",
        "issn": "0028-0836",
        "publisher": "Nature Publishing Group",
        "publication": "Nature",
        "publication_date": "2012-01-05",
        "series_number": "7379",
        "volume": "481",
        "issue": "7379",
        "pages": "58-61"
    },
    {
        "id": "authors:6gf4s-9gm33",
        "collection": "authors",
        "collection_id": "6gf4s-9gm33",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20120125-085020111",
        "type": "article",
        "title": "The Relative Humidity in an Isentropic Advection\u2013Condensation Model: Limited Poleward Influence and Properties of Subtropical Minima",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Lamquin",
                "given_name": "Nicolas",
                "clpid": "Lamquin-N"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Singh",
                "given_name": "Martin S.",
                "clpid": "Singh-M-S"
            }
        ],
        "abstract": "An idealized model of advection and condensation of water vapor is considered as a representation of processes influencing the humidity distribution along isentropic surfaces in the free troposphere. Results are presented for how the mean relative humidity distribution varies in response to changes in the distribution of saturation specific humidity and in the amplitude of a tropical moisture source. Changes in the tropical moisture source are found to have little effect on the relative humidity poleward of the subtropical minima, suggesting a lack of poleward influence despite much greater water vapor concentrations at lower latitudes. The subtropical minima in relative humidity are found to be located just equatorward of the inflection points of the saturation specific humidity profile along the isentropic surface. The degree of mean subsaturation is found to vary with the magnitude of the meridional gradient of saturation specific humidity when other parameters are held fixed.\n\nThe atmospheric relevance of these results is investigated by comparison with the positions of the relative humidity minima in reanalysis data and by examining poleward influence of relative humidity in simulations with an idealized general circulation model. It is suggested that the limited poleward influence of relative humidity may constrain the propagation of errors in simulated humidity fields.",
        "doi": "10.1175/JAS-D-11-067.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2011-12",
        "series_number": "12",
        "volume": "68",
        "issue": "12",
        "pages": "3079-3093"
    },
    {
        "id": "authors:v5zbw-m7216",
        "collection": "authors",
        "collection_id": "v5zbw-m7216",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111219-092158853",
        "type": "article",
        "title": "Convective Generation of Equatorial Superrotation in Planetary Atmospheres",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "In rapidly rotating planetary atmospheres that are heated from below, equatorial superrotation can occur through convective generation of equatorial Rossby waves. If the heating from below is sufficiently strong that convection penetrates into the upper troposphere, then the convection generates equatorial Rossby waves, which can induce the equatorward angular momentum transport necessary for superrotation. This paper investigates the conditions under which the convective generation of equatorial Rossby waves and their angular momentum transport lead to superrotation. It also addresses how the strength and width of superrotating equatorial jets are controlled.\n\nIn simulations with an idealized general circulation model (GCM), the relative roles of baroclinicity, heating from below, and bottom drag are explored systematically. Equatorial superrotation generally occurs when the heating from below is sufficiently strong. However, the threshold heating at which the transition to superrotation occurs increases as the baroclinicity or the bottom drag increases. The greater the baroclinicity is, the stronger the angular momentum transport out of low latitudes by baroclinic eddies of extratropical origin. This competes with the angular momentum transport toward the equator by convectively generated Rossby waves and thus can inhibit a transition to superrotation. Equatorial bottom drag damps both the mean zonal flow and convectively generated Rossby waves, weakening the equatorward angular momentum transport as the drag increases; this can also inhibit a transition to superrotation. The strength of superrotating equatorial jets scales approximately with the square of their width. When they are sufficiently strong, their width, in turn, scales with the equatorial Rossby radius and thus depends on the thermal stratification of the equatorial atmosphere.\n\nThe results have broad implications for planetary atmospheres, particularly for how superrotation can be generated in giant planet atmospheres and in terrestrial atmospheres in warm climates.",
        "doi": "10.1175/JAS-D-10-05013.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2011-11",
        "series_number": "11",
        "volume": "68",
        "issue": "11",
        "pages": "2742-2756"
    },
    {
        "id": "authors:athzm-a7c30",
        "collection": "authors",
        "collection_id": "athzm-a7c30",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111121-101315922",
        "type": "article",
        "title": "Consistent Changes in the Sea Ice Seasonal Cycle in Response to Global Warming",
        "author": [
            {
                "family_name": "Eisenman",
                "given_name": "Ian",
                "clpid": "Eisenman-I"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Battisti",
                "given_name": "David S.",
                "orcid": "0000-0003-4871-1293",
                "clpid": "Battisti-D-S"
            },
            {
                "family_name": "Bitz",
                "given_name": "Cecilia M.",
                "clpid": "Bitz-C-M"
            }
        ],
        "abstract": "The Northern Hemisphere sea ice cover has diminished rapidly in recent years and is projected to continue to diminish in the future. The year-to-year retreat of Northern Hemisphere sea ice extent is faster in summer than winter, which has been identified as one of the most striking features of satellite observations as well as of state-of-the-art climate model projections. This is typically understood to imply that the sea ice cover is most sensitive to climate forcing in summertime, and previous studies have explained this by calling on factors such as the surface albedo feedback. In the Southern Hemisphere, however, it is the wintertime sea ice extent that retreats fastest in climate model projections. Here, it is shown that the interhemispheric differences in the model projections can be attributed to differences in coastline geometry, which constrain where sea ice can occur. After accounting for coastline geometry, it is found that the sea ice changes simulated in both hemispheres in most climate models are consistent with sea ice retreat being fastest in winter in the absence of landmasses. These results demonstrate that, despite the widely differing rates of ice retreat among climate model projections, the seasonal structure of the sea ice retreat is robust among the models and is uniform in both hemispheres.",
        "doi": "10.1175/2011JCLI4051.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2011-10-15",
        "series_number": "20",
        "volume": "24",
        "issue": "20",
        "pages": "5325-5335"
    },
    {
        "id": "authors:zbyr2-nnq27",
        "collection": "authors",
        "collection_id": "zbyr2-nnq27",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111114-153036980",
        "type": "article",
        "title": "Downstream Self-Destruction of Storm Tracks",
        "author": [
            {
                "family_name": "Kaspi",
                "given_name": "Yohai",
                "orcid": "0000-0003-4089-0020",
                "clpid": "Kaspi-Y"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The Northern Hemisphere storm tracks have maximum intensity over the Pacific and Atlantic basins; their intensity is reduced over the continents downstream. Here, simulations with an idealized aquaplanet general circulation model are used to demonstrate that even without continents, storm tracks have a self-determined longitudinal length scale. Their length is controlled primarily by the planetary rotation rate and is similar to that of Earth's storm tracks for Earth's rotation rate. Downstream, storm tracks self-destruct: the downstream eddy kinetic energy is lower than it would be without the zonal asymmetries that cause localized storm tracks. Likely involved in the downstream self-destruction of storm tracks are the energy fluxes associated with them. The zonal asymmetries that cause localized storm tracks enhance the energy transport through the generation of stationary eddies, and this leads to a reduced baroclinicity that persists far downstream of the eddy kinetic energy maxima.",
        "doi": "10.1175/JAS-D-10-05002.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2011-10",
        "series_number": "10",
        "volume": "68",
        "issue": "10",
        "pages": "2459-2464"
    },
    {
        "id": "authors:0hnxd-13502",
        "collection": "authors",
        "collection_id": "0hnxd-13502",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20111012-074304154",
        "type": "article",
        "title": "Changes in Zonal Surface Temperature Gradients and Walker Circulations in a Wide Range of Climates",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Variations in zonal surface temperature gradients and zonally asymmetric tropical overturning circulations (Walker circulations) are examined over a wide range of climates simulated with an idealized atmospheric general circulation model (GCM). The asymmetry in the tropical climate is generated by an imposed ocean energy flux, which does not vary with climate. The range of climates is simulated by modifying the optical thickness of an idealized longwave absorber (representing greenhouse gases).\n\nThe zonal surface temperature gradient in low latitudes generally decreases as the climate warms in the idealized GCM simulations. A scaling relationship based on a two-term balance in the surface energy budget accounts for the changes in the zonally asymmetric component of the GCM-simulated surface temperature.\n\nThe Walker circulation weakens as the climate warms in the idealized simulations, as it does in comprehensive simulations of climate change. The wide range of climates allows a systematic test of energetic arguments that have been proposed to account for these changes in the tropical circulation. The analysis shows that a scaling estimate based on changes in the hydrological cycle (precipitation rate and saturation specific humidity) accounts for the simulated changes in the Walker circulation. However, it must be evaluated locally, with local precipitation rates. If global-mean quantities are used, the scaling estimate does not generally account for changes in the Walker circulation, and the extent to which it does is the result of compensating errors in changes in precipitation and saturation specific humidity that enter the scaling estimate.",
        "doi": "10.1175/2011JCLI4042.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2011-09",
        "series_number": "17",
        "volume": "24",
        "issue": "17",
        "pages": "4757-4768"
    },
    {
        "id": "authors:75rtb-xba43",
        "collection": "authors",
        "collection_id": "75rtb-xba43",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110520-080425147",
        "type": "article",
        "title": "Sources of variations in total column carbon dioxide",
        "author": [
            {
                "family_name": "Keppel-Aleks",
                "given_name": "G.",
                "clpid": "Keppel-Aleks-G"
            },
            {
                "family_name": "Wennberg",
                "given_name": "P. O.",
                "orcid": "0000-0002-6126-3854",
                "clpid": "Wennberg-P-O"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Observations of gradients in the total CO_2 column,\n(CO2), are expected to provide improved constraints\non surface fluxes of CO_2. Here we use a general circulation\nmodel with a variety of prescribed carbon fluxes to investigate how variations in (CO_2) arise. On diurnal scales, variations are small and are forced by both local fluxes and advection. On seasonal scales, gradients are set by the north-south flux distribution. On synoptic scales, variations arise due to large-scale eddy-driven disturbances of the meridional gradient. In this case, because variations in (CO_2) are tied to synoptic\nactivity, significant correlations exist between (CO_2)\nand dynamical tracers. We illustrate how such correlations\ncan be used to describe the north-south gradients of (CO_2)\nand the underlying fluxes on continental scales. These simulations suggest a novel analysis framework for using column observations in carbon cycle science.",
        "doi": "10.5194/acp-11-3581-2011",
        "issn": "1680-7316",
        "publisher": "European Geosciences Union",
        "publication": "Atmospheric Chemistry and Physics",
        "publication_date": "2011-04-18",
        "series_number": "8",
        "volume": "11",
        "issue": "8",
        "pages": "3581-3593"
    },
    {
        "id": "authors:y8dqt-ffg65",
        "collection": "authors",
        "collection_id": "y8dqt-ffg65",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110502-105810785",
        "type": "article",
        "title": "Response of the Hadley Circulation to Climate Change in an Aquaplanet GCM Coupled to a Simple Representation of Ocean Heat Transport",
        "author": [
            {
                "family_name": "Levine",
                "given_name": "Xavier J.",
                "clpid": "Levine-X-J"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "It is unclear how the width and strength of the Hadley circulation are controlled and how they respond to climate changes. Simulations of global warming scenarios with comprehensive climate models suggest the Hadley circulation may widen and weaken as the climate warms. But these changes are not quantitatively consistent among models, and how they come about is not understood. Here, a wide range of climates is simulated with an idealized moist general circulation model (GCM) coupled to a simple representation of ocean heat transport, in order to place past and possible future changes in the Hadley circulation into a broader context and to investigate the mechanisms responsible for them.\n\nBy comparison of simulations with and without ocean heat transport, it is shown that it is essential to take low-latitude ocean heat transport and its coupling to wind stress into account to obtain Hadley circulations in a dynamical regime resembling Earth's, particularly in climates resembling present-day Earth's and colder. As the optical thickness of an idealized longwave absorber in the simulations is increased and the climate warms, the Hadley circulation strengthens in colder climates and weakens in warmer climates; it has maximum strength in a climate close to present-day Earth's. In climates resembling present-day Earth's and colder, the Hadley circulation strength is largely controlled by the divergence of angular momentum fluxes associated with eddies of midlatitude origin; the latter scale with the mean available potential energy in midlatitudes. The importance of these eddy momentum fluxes for the Hadley circulation strength gradually diminishes as the climate warms. The Hadley circulation generally widens as the climate warms, but at a modest rate that depends sensitively on how it is determined.",
        "doi": "10.1175/2010JAS3553.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2011-04",
        "series_number": "4",
        "volume": "68",
        "issue": "4",
        "pages": "769-783"
    },
    {
        "id": "authors:q7ggm-ja377",
        "collection": "authors",
        "collection_id": "q7ggm-ja377",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20110419-142949447",
        "type": "article",
        "title": "Winter cold of eastern continental boundaries induced by warm ocean waters",
        "author": [
            {
                "family_name": "Kaspi",
                "given_name": "Yohai",
                "orcid": "0000-0003-4089-0020",
                "clpid": "Kaspi-Y"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "In winter, northeastern North America and northeastern Asia are both colder than other regions at similar latitudes. This has been attributed to the effects of stationary weather systems set by elevated terrain (orography), and to a lack of maritime influences from the prevailing westerly winds. However, the differences in extent and orography between the two continents suggest that further mechanisms are involved. Here we show that this anomalous winter cold can result in part from westward radiation of large-scale atmospheric waves\u2014nearly stationary Rossby waves\u2014generated by heating of the atmosphere over warm ocean waters. We demonstrate this mechanism using simulations with an idealized general circulation model, with which we show that the extent of the cold region is controlled by properties of Rossby waves, such as their group velocity and its dependence on the planetary rotation rate. Our results show that warm ocean waters contribute to the contrast in mid-latitude winter temperatures between eastern and western continental boundaries not only by warming western boundaries, but also by cooling eastern boundaries.",
        "doi": "10.1038/nature09924",
        "issn": "0028-0836",
        "publisher": "Nature Publishing Group",
        "publication": "Nature",
        "publication_date": "2011-03-31",
        "series_number": "7340",
        "volume": "471",
        "issue": "7340",
        "pages": "621-624"
    },
    {
        "id": "authors:vaa73-6e980",
        "collection": "authors",
        "collection_id": "vaa73-6e980",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20101220-141832153",
        "type": "article",
        "title": "Mechanisms of Jet Formation on the Giant Planets",
        "author": [
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The giant planet atmospheres exhibit alternating prograde (eastward) and retrograde (westward) jets of different speeds and widths, with an equatorial jet that is prograde on Jupiter and Saturn and retrograde on Uranus and Neptune. The jets are variously thought to be driven by differential radiative heating of the upper atmosphere or by intrinsic heat fluxes emanating from the deep interior. However, existing models cannot account for the different flow configurations on the giant planets in an energetically consistent manner. Here a three-dimensional general circulation model is used to show that the different flow configurations can be reproduced by mechanisms universal across the giant planets if differences in their radiative heating and intrinsic heat fluxes are taken into account. Whether the equatorial jet is prograde or retrograde depends on whether the deep intrinsic heat fluxes are strong enough that convection penetrates into the upper troposphere and generates strong equatorial Rossby waves there. Prograde equatorial jets result if convective Rossby wave generation is strong and low-latitude angular momentum flux divergence owing to baroclinic eddies generated off the equator is sufficiently weak (Jupiter and Saturn). Retrograde equatorial jets result if either convective Rossby wave generation is weak or absent (Uranus) or low-latitude angular momentum flux divergence owing to baroclinic eddies is sufficiently strong (Neptune). The different speeds and widths of the off-equatorial jets depend, among other factors, on the differential radiative heating of the atmosphere and the altitude of the jets, which are vertically sheared. The simulations have closed energy and angular momentum balances that are consistent with observations of the giant planets. They exhibit temperature structures closely resembling those observed and make predictions about as yet unobserved aspects of flow and temperature structures.",
        "doi": "10.1175/2010JAS3492.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2010-11",
        "series_number": "11",
        "volume": "67",
        "issue": "11",
        "pages": "3652-3672"
    },
    {
        "id": "authors:bzmwz-e6397",
        "collection": "authors",
        "collection_id": "bzmwz-e6397",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100803-093823508",
        "type": "article",
        "title": "Water vapor and the dynamics of climate changes",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Levine",
                "given_name": "Xavier J.",
                "clpid": "Levine-X-J"
            }
        ],
        "abstract": "Water vapor is not only Earth's dominant greenhouse gas. Through the release of latent heat when it condenses, it also plays an active role in dynamic processes that shape the global circulation of the atmosphere and thus climate. Here we present an overview of how latent heat release affects atmosphere dynamics in a broad range of climates, ranging from extremely cold to extremely warm. Contrary to widely held beliefs, atmospheric circulation statistics can change nonmonotonically with global-mean surface temperature, in part because of dynamic effects of water vapor. For example, the strengths of the tropical Hadley circulation and of zonally asymmetric tropical circulations, as well as the kinetic energy of extratropical baroclinic eddies, can be lower than they presently are both in much warmer climates and in much colder climates. We discuss how latent heat release is implicated in such circulation changes, particularly through its effect on the atmospheric static stability, and we illustrate the circulation changes through simulations with an idealized general circulation model. This allows us to explore a continuum of climates, to constrain macroscopic laws governing this climatic continuum, and to place past and possible future climate changes in a broader context.",
        "doi": "10.1029/2009RG000302",
        "issn": "8755-1209",
        "publisher": "American Geophysical Union",
        "publication": "Reviews of Geophysics",
        "publication_date": "2010-07-02",
        "volume": "48",
        "pages": "Art. No. RG3001"
    },
    {
        "id": "authors:tpxm3-0f224",
        "collection": "authors",
        "collection_id": "tpxm3-0f224",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100629-085126837",
        "type": "article",
        "title": "Regime Transitions of Steady and Time-Dependent Hadley Circulations:\n Comparison of Axisymmetric and Eddy-Permitting Simulations",
        "author": [
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Steady-state and time-dependent Hadley circulations are investigated with an idealized dry GCM, in which\nthermal forcing is represented as relaxation of temperatures toward a radiative-equilibrium state. The latitude\n\u03d5_0 of maximum radiative-equilibrium temperature is progressively displaced off the equator or varied in time\nto study how the Hadley circulation responds to seasonally varying forcing; axisymmetric simulations are\ncompared with eddy-permitting simulations. In axisymmetric steady-state simulations, the Hadley circulations\nfor all \u03d5_0 approach the nearly inviscid, angular-momentum-conserving limit, despite the presence of\nfinite vertical diffusion of momentum and dry static energy. In contrast, in corresponding eddy-permitting\nsimulations, the Hadley circulations undergo a regime transition as \u03d5_0 is increased, from an equinox regime\n(small \u03d5_0) in which eddy momentumfluxes strongly influence both Hadley cells to a solstice regime (large \u03d5_0)\nin which the cross-equatorial winter Hadley cell more closely approaches the angular-momentum-conserving\nlimit. In axisymmetric time-dependent simulations, the Hadley cells undergo transitions between a linear\nequinox regime and a nonlinear, nearly angular-momentum-conserving solstice regime. Unlike in the eddypermitting\nsimulations, time tendencies of the zonal wind play a role in the dynamics of the transitions in\nthe axisymmetric simulation. Nonetheless, the axisymmetric transitions are similar to those in the eddypermitting\nsimulations in that the role of the nonlinear mean momentum flux divergence in the zonal momentum\nbudget shifts from marginal in the equinox regime to dominant in the solstice regime. As in the\neddy-permitting simulations, a mean-flow feedback\u2014involving the upper-level zonal winds, the lower-level\ntemperature gradient, and the poleward boundary of the cross-equatorial Hadley cell\u2014makes it possible for\nthe circulation fields to change at the transition more rapidly than can be explained by the steady-state response\nto the thermal forcing. However, the regime transitions in the axisymmetric simulations are less sharp\nthan those in the eddy-permitting simulations because eddy\u2013mean flow feedbacks in the eddy-permitting\nsimulations additionally sharpen the transitions.",
        "doi": "10.1175/2009JAS3294.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2010-05",
        "series_number": "5",
        "volume": "67",
        "issue": "5",
        "pages": "1643-1654"
    },
    {
        "id": "authors:vhdgr-khw60",
        "collection": "authors",
        "collection_id": "vhdgr-khw60",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-155139882",
        "type": "article",
        "title": "Atmospheric Dynamics of Earth-Like Tidally Locked Aquaplanets",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "We present simulations of atmospheres of Earth-like aquaplanets that are tidally locked to their star, that is, planets whose orbital period is equal to the rotation period about their spin axis, so that one side always faces the star and the other side is always dark. Such simulations are of interest in the study of tidally locked terrestrial exoplanets and as illustrations of how planetary rotation and the insolation distribution shape climate. As extreme cases illustrating the effects of slow and rapid rotation, we consider planets with rotation periods equal to one current Earth year and one current Earth day. The dynamics responsible for the surface climate (e.g., winds, temperature, precipitation) and the general circulation of the atmosphere are discussed in light of existing theories of atmospheric circulations. For example, as expected from the increasing importance of Coriolis accelerations relative to inertial accelerations as the rotation rate increases, the winds are approximately isotropic and divergent at leading order in the slowly rotating atmosphere but are predominantly zonal and rotational in the rapidly rotating atmosphere. Free-atmospheric horizontal temperature variations in the slowly rotating atmosphere are generally weaker than in the rapidly rotating atmosphere. Interestingly, the surface temperature on the night side of the planets does not fall below \u223c240 K in either the rapidly or slowly rotating atmosphere; that is, heat transport from the day side to the night side of the planets efficiently reduces temperature contrasts in either case. Rotational waves and eddies shape the distribution of winds, temperature, and precipitation in the rapidly rotating atmosphere; in the slowly rotating atmosphere, these distributions are controlled by simpler divergent circulations. Both the slowly and rapidly rotating atmospheres exhibit equatorial superrotation. Systematic variation of the planetary rotation rate shows that the equatorial superrotation varies non-monotonically with rotation rate, whereas the surface temperature contrast between the day side and the night side does not vary strongly with changes in rotation rate.",
        "doi": "10.3894/JAMES.2010.2.13",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2010-04",
        "series_number": "4",
        "volume": "2",
        "issue": "4",
        "pages": "Art. No. 13"
    },
    {
        "id": "authors:ytaaa-9yz32",
        "collection": "authors",
        "collection_id": "ytaaa-9yz32",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20100217-112336766",
        "type": "article",
        "title": "The Maintenance of the Relative Humidity of the Subtropical Free Troposphere",
        "author": [
            {
                "family_name": "Couhert",
                "given_name": "Alexandre",
                "clpid": "Couhert-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Li",
                "given_name": "Juilin",
                "clpid": "Li-J"
            },
            {
                "family_name": "Waliser",
                "given_name": "Duane E.",
                "clpid": "Waliser-D-E"
            },
            {
                "family_name": "Tompkins",
                "given_name": "Adrian M.",
                "clpid": "Tompkins-A-M"
            }
        ],
        "abstract": "The relative importance of different processes in the water vapor balance of the troposphere is assessed, using high-resolution hindcast data from the ECMWF Integrated Forecast System (IFS) for December\u2013February 1998/99 interpolated to isentropic coordinates. The focus is on elucidating the processes that maintain the relative humidity of the subtropical free troposphere. The dominant drying process in the subtropical free troposphere is cross-isentropic subsidence driven by radiative cooling. In some subtropical regions [e.g., over continents in the Southern (summer) Hemisphere and over western portions of ocean basins in the Northern (winter) Hemisphere], drying by radiative subsidence is partially offset or overcompensated by moistening by cross-isentropic dynamic transport of water vapor from the surface upward (e.g., in convection). Any resultant net drying or moistening of the subtropical free troposphere by cross-isentropic motions is regionally primarily balanced by isentropic mean and eddy transport of water vapor from moister into drier regions. Isentropic transport redistributes water vapor within the subtropics and moderates relative humidity contrasts; however, it does not consistently lead to a substantial net import or export of water vapor into or out of the subtropics.",
        "doi": "10.1175/2009JCLI2952.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2010-01",
        "series_number": "2",
        "volume": "23",
        "issue": "2",
        "pages": "390-403"
    },
    {
        "id": "authors:mbw63-cyt33",
        "collection": "authors",
        "collection_id": "mbw63-cyt33",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20091124-113114811",
        "type": "article",
        "title": "Scaling of Precipitation Extremes over a Wide Range of Climates Simulated with an Idealized GCM",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Extremes of precipitation are examined in a wide range of climates simulated with an idealized aquaplanet GCM. The high percentiles of daily precipitation increase as the climate warms. Their fractional rate of increase with global-mean surface temperature is generally similar to or greater than that of mean precipitation, but it is less than that of atmospheric (column) water vapor content. A simple scaling is introduced for precipitation extremes that accounts for their behavior by including the effects of changes in the moist-adiabatic lapse rate, the circulation strength, and the temperature when the extreme events occur. The effects of changes in the moist-adiabatic lapse rate and circulation strength on precipitation extremes are important globally, whereas the difference in the mean temperature and the temperature at which precipitation extremes occur is important only at middle to high latitudes.",
        "doi": "10.1175/2009JCLI2701.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2009-11",
        "series_number": "21",
        "volume": "22",
        "issue": "21",
        "pages": "5676-5685"
    },
    {
        "id": "authors:ged8k-xpa53",
        "collection": "authors",
        "collection_id": "ged8k-xpa53",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20090911-153558204",
        "type": "article",
        "title": "The physical basis for increases in precipitation extremes in simulations of 21st-century climate change",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Global warming is expected to lead to a large increase in atmospheric water vapor content and to changes in the hydrological cycle, which include an intensification of precipitation extremes. The intensity of precipitation extremes is widely held to increase proportionately to the increase in atmospheric water vapor content. Here, we show that this is not the case in 21st-century climate change scenarios simulated with climate models. In the tropics, precipitation extremes are not simulated reliably and do not change consistently among climate models; in the extratropics, they consistently increase more slowly than atmospheric water vapor content. We give a physical basis for how precipitation extremes change with climate and show that their changes depend on changes in the moist-adiabatic temperature lapse rate, in the upward velocity, and in the temperature when precipitation extremes occur. For the tropics, the theory suggests that improving the simulation of upward velocities in climate models is essential for improving predictions of precipitation extremes; for the extratropics, agreement with theory and the consistency among climate models increase confidence in the robustness of predictions of precipitation extremes under climate change.",
        "doi": "10.1073/pnas.0907610106",
        "pmcid": "PMC2736420",
        "issn": "0027-8424",
        "publisher": "National Academy of Sciences",
        "publication": "Proceedings of the National Academy of Sciences of the United States of America",
        "publication_date": "2009-09-01",
        "series_number": "35",
        "volume": "106",
        "issue": "35",
        "pages": "14773-14777"
    },
    {
        "id": "authors:fr5g9-jg977",
        "collection": "authors",
        "collection_id": "fr5g9-jg977",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20090828-231032364",
        "type": "article",
        "title": "Storms in the tropics of Titan",
        "author": [
            {
                "family_name": "Schaller",
                "given_name": "E. L.",
                "clpid": "Schaller-E-L"
            },
            {
                "family_name": "Roe",
                "given_name": "H. G.",
                "clpid": "Roe-H-G"
            },
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Brown",
                "given_name": "M. E.",
                "orcid": "0000-0002-8255-0545",
                "clpid": "Brown-M-E"
            }
        ],
        "abstract": "Methane clouds, lakes and most fluvial features on Saturn's moon Titan have been observed in the moist high latitudes while the tropics have been nearly devoid of convective clouds and have shown an abundance of wind-carved surface features like dunes. The presence of small-scale channels and dry riverbeds near the equator observed by the Huygens probe at latitudes thought incapable of supporting convection (and thus strong rain) has been suggested to be due to geological seepage or other mechanisms not related to precipitation. Here we report the presence of bright, transient, tropospheric clouds in tropical latitudes. We find that the initial pulse of cloud activity generated planetary waves that instigated cloud activity at other latitudes across Titan that had been cloud-free for at least several years. These observations show that convective pulses at one latitude can trigger short-term convection at other latitudes, even those not generally considered capable of supporting convection, and may also explain the presence of methane-carved rivers and channels near the Huygens landing site.",
        "doi": "10.1038/nature08193",
        "issn": "0028-0836",
        "publisher": "Nature Publishing Group",
        "publication": "Nature",
        "publication_date": "2009-08-13",
        "series_number": "7257",
        "volume": "460",
        "issue": "7257",
        "pages": "873-875"
    },
    {
        "id": "authors:dvf87-7r657",
        "collection": "authors",
        "collection_id": "dvf87-7r657",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20090821-151334152",
        "type": "article",
        "title": "Scales of Linear Baroclinic Instability and Macroturbulence in Dry Atmospheres",
        "author": [
            {
                "family_name": "Merlis",
                "given_name": "Timothy M.",
                "clpid": "Merlis-T-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Linear stability analyses are performed on a wide range of mean flows simulated with a dry idealized general circulation model. The zonal length scale of the linearly most unstable waves is similar to the Rossby radius. It is also similar to the energy-containing zonal length scale in statistically steady states of corresponding nonlinear simulations. The meridional length scale of the linearly most unstable waves is generally smaller than the energy-containing meridional length scale in the corresponding nonlinear simulations. The growth rate of the most unstable waves increases with increasing Eady growth rate, but the scaling relationship is not linear in general. The available potential energy and barotropic and baroclinic kinetic energies of the linearly most unstable waves scale linearly with each other, with similar partitionings among the energy forms as in the corresponding nonlinear simulations. These results show that the mean flows in the nonlinear simulations are baroclinically unstable, yet there is no substantial inverse cascade of barotropic eddy kinetic energy from the baroclinic generation scale to larger scales, even in strongly unstable flows. Some aspects of the nonlinear simulations, such as partitionings among eddy energies, can be understood on the basis of linear stability analyses; for other aspects, such as the structure of heat and momentum fluxes, nonlinear modifications of the waves are important.",
        "doi": "10.1175/2008JAS2884.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2009-06",
        "series_number": "6",
        "volume": "66",
        "issue": "6",
        "pages": "1821-1833"
    },
    {
        "id": "authors:1ka92-p8811",
        "collection": "authors",
        "collection_id": "1ka92-p8811",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20161004-105301466",
        "type": "article",
        "title": "Single-layer axisymmetric model for a Hadley circulation with parameterized eddy momentum forcing",
        "author": [
            {
                "family_name": "Sobel",
                "given_name": "Adam H.",
                "clpid": "Sobel-A-H"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "An axisymmetric single-layer model is used to study interactions of the Hadley circulation with extratropical eddies. Eddy momentum fluxes are parameterized using a simple closure motivated by calculations with an idealized dry general circulation model (GCM). Calculations are performed in which the heating is parameterized as Newtonian relaxation of temperatures toward a prescribed radiative-convective equilibrium (RCE) state. The latitude at which the maximum RCE temperature occurs is varied to represent seasonal variations. In the axisymmetric model, as in the GCM, qualitative changes in the zonal momentum budget occur as the RCE temperature maximum moves away from the equator past a threshold latitude. For RCE temperature maxima closer to the equator, eddy momentum fluxes play a dominant role in the zonal momentum budget, nonlinearity is weak, and the meridional circulation is a weak function of the degree of asymmetry about the equator. For RCE temperature maxima sufficiently far from the equator, the zonal momentum budget becomes more nonlinear, angular momentum is more nearly conserved, and the circulation is a stronger function of the degree of asymmetry about the equator. Since the axisymmetric model can capture this behavior while being much simpler than the GCM, it may be a useful step towards a more comprehensive theory of the zonal-mean general circulation.",
        "doi": "10.3894/JAMES.2009.1.10",
        "issn": "1942-2466",
        "publisher": "American Geophysical Union",
        "publication": "Journal of Advances in Modeling Earth Systems",
        "publication_date": "2009-03",
        "series_number": "3",
        "volume": "1",
        "issue": "3",
        "pages": "Art. No. 10"
    },
    {
        "id": "authors:qkzd4-nq324",
        "collection": "authors",
        "collection_id": "qkzd4-nq324",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20090709-092656156",
        "type": "article",
        "title": "Formation of jets and equatorial superrotation on Jupiter",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Liu",
                "given_name": "Junjun",
                "clpid": "Liu-Junjun"
            }
        ],
        "abstract": "The zonal flow in Jupiter's upper troposphere is organized into alternating retrograde and prograde jets, with\na prograde (superrotating) jet at the equator. Existing models posit as the driver of the flow either differential\nradiative heating of the atmosphere or intrinsic heat fluxes emanating from the deep interior; however, they do\nnot reproduce all large-scale features of Jupiter's jets and thermal structure. Here it is shown that the difficulties\nin accounting for Jupiter's jets and thermal structure resolve if the effects of differential radiative\nheating and intrinsic heat fluxes are considered together, and if upper-tropospheric dynamics are linked to a\nmagnetohydrodynamic(MHD)drag that acts deep in the atmosphere and affects the zonal flow away from but\nnot near the equator. Baroclinic eddies generated by differential radiative heating can account for the off-equatorial\njets; meridionally propagating equatorial Rossby waves generated by intrinsic convective heat\nfluxes can account for the equatorial superrotation. The zonal flow extends deeply into the atmosphere, with its\nspeed changing with depth, away from the equator up to depths at which the MHD drag acts. The theory is\nsupported by simulations with an energetically consistent general circulation model of Jupiter's outer atmosphere.\nA simulation that incorporates differential radiative heating and intrinsic heat fluxes reproduces\nJupiter's observed jets and thermal structure and makes testable predictions about as yet unobserved aspects\nthereof. A control simulation that incorporates only differential radiative heating but not intrinsic heat fluxes\nproduces off-equatorial jets but no equatorial superrotation; another control simulation that incorporates only\nintrinsic heat fluxes but not differential radiative heating produces equatorial superrotation but no off-equatorial\njets. The proposed mechanisms for the formation of jets and equatorial superrotation likely act\nin the atmospheres of all giant planets.",
        "doi": "10.1175/2008JAS2798.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2009-03",
        "series_number": "3",
        "volume": "66",
        "issue": "3",
        "pages": "579-601"
    },
    {
        "id": "authors:jmkk6-cxh43",
        "collection": "authors",
        "collection_id": "jmkk6-cxh43",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:KORgrl08",
        "type": "article",
        "title": "Extent of Hadley circulations in dry atmospheres",
        "author": [
            {
                "family_name": "Korty",
                "given_name": "Robert L.",
                "clpid": "Korty-R-L"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The subtropical terminus of the Hadley circulation is interpreted as the latitude poleward of which vertical wave activity fluxes (meridional eddy entropy fluxes) become sufficiently deep to reach the upper troposphere. This leads to a sign change of the upper-tropospheric divergence of meridional wave activity fluxes (convergence of meridional eddy angular momentum fluxes) and marks the transition from the tropical Hadley cell to the extratropical Ferrel cell. A quantitative formulation for determining the depth of vertical wave activity fluxes and thus the terminus of the Hadley circulation is proposed based on the supercriticality, a measure of the slope of isentropes. The supercriticality assumes an approximately constant value at the terminus of the Hadley circulation in a series of simulations with an idealized dry general circulation model. However, it is unclear how to generalize this supercriticality-based formulation to moist atmospheres.",
        "doi": "10.1029/2008GL035847",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2008-12-02",
        "series_number": "23",
        "volume": "35",
        "issue": "23",
        "pages": "L23803"
    },
    {
        "id": "authors:vspp0-w8j70",
        "collection": "authors",
        "collection_id": "vspp0-w8j70",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:OGOjc08b",
        "type": "article",
        "title": "Energy of Midlatitude Transient Eddies in Idealized Simulations of Changed Climates",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "As the climate changes, changes in static stability, meridional temperature gradients, and availability of moisture for latent heat release may exert competing effects on the energy of midlatitude transient eddies. This paper examines how the eddy kinetic energy in midlatitude baroclinic zones responds to changes in radiative forcing in simulations with an idealized moist general circulation model. In a series of simulations in which the optical thickness of the longwave absorber is varied over a wide range, the eddy kinetic energy has a maximum for a climate with mean temperature similar to that of present-day earth, with significantly smaller values both for warmer and for colder climates. In a series of simulations in which the meridional insolation gradient is varied, the eddy kinetic energy increases monotonically with insolation gradient. In both series of simulations, the eddy kinetic energy scales approximately linearly with the dry mean available potential energy averaged over the baroclinic zones. Changes in eddy kinetic energy can therefore be related to the changes in the atmospheric thermal structure that affect the mean available potential energy.",
        "doi": "10.1175/2008JCLI2099.1",
        "issn": "0894-8755",
        "publisher": "american met",
        "publication": "Journal of Climate",
        "publication_date": "2008-11-15",
        "series_number": "22",
        "volume": "21",
        "issue": "22",
        "pages": "5797-5806"
    },
    {
        "id": "authors:w8n94-c4d80",
        "collection": "authors",
        "collection_id": "w8n94-c4d80",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas08c",
        "type": "article",
        "title": "Moist Convection and the Thermal Stratification of the Extratropical Troposphere",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            }
        ],
        "abstract": "Simulations with an aquaplanet general circulation model show that sensible and latent heat transport by large-scale eddies influences the extratropical thermal stratification over a wide range of climates, even in relatively warm climates with small meridional surface temperature gradients. Variations of the lapse rate toward which the parameterized moist convection in the model relaxes atmospheric temperature profiles demonstrate that the convective lapse rate only marginally affects the extratropical thermal stratification in Earth-like and colder climates. In warmer climates, the convective lapse rate does affect the extratropical thermal stratification, but the effect is still smaller than would be expected if moist convection alone controlled the thermal stratification. A theory for how large-scale eddies modify the thermal stratification of dry atmospheres is consistent with the simulation results for colder climates. For warmer and moister climates, however, theories and heuristics that have been proposed to account for the extratropical thermal stratification are not consistent with the simulation results. Theories for the extratropical thermal stratification will generally have to take transport of sensible and latent heat by large-scale eddies into account, but moist convection may only need to be taken into account regionally and in sufficiently warm climates.",
        "doi": "10.1175/2008JAS2652.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2008-11",
        "series_number": "11",
        "volume": "65",
        "issue": "11",
        "pages": "3571-3583"
    },
    {
        "id": "authors:bd2ae-7qf61",
        "collection": "authors",
        "collection_id": "bd2ae-7qf61",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:OGOjc08a",
        "type": "article",
        "title": "The Hydrological Cycle over a Wide Range of Climates Simulated with an Idealized GCM",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "A wide range of hydrological cycles and general circulations was simulated with an idealized general circulation model (GCM) by varying the optical thickness of the longwave absorber. While the idealized GCM does not capture the full complexity of the hydrological cycle, the wide range of climates simulated allows the systematic development and testing of theories of how precipitation and moisture transport change as the climate changes. The simulations show that the character of the response of the hydrological cycle to variations in longwave optical thickness differs in different climate regimes. \n\nThe global-mean precipitation increases linearly with surface temperature for colder climates, but it asymptotically approaches a maximum at higher surface temperatures. The basic features of the precipitation\u2013temperature relation, including the rate of increase in the linear regime, are reproduced in radiative\u2013convective equilibrium simulations. Energy constraints partially account for the precipitation\u2013temperature relation but are not quantitatively accurate. \n\nLarge-scale condensation is most important in the midlatitude storm tracks, and its behavior is accounted for using a stochastic model of moisture advection and condensation. The precipitation associated with large-scale condensation does not scale with mean specific humidity, partly because the condensation region moves upward and meridionally as the climate warms, and partly because the mean condensation rate depends on isentropic specific humidity gradients, which do not scale with the specific humidity itself. \n\nThe local water vapor budget relates local precipitation to evaporation and meridional moisture fluxes, whose scaling in the subtropics and extratropics is examined. A delicate balance between opposing changes in evaporation and moisture flux divergence holds in the subtropical dry zones. The extratropical precipitation maximum follows the storm track in warm climates but lies equatorward of the storm track in cold climates.",
        "doi": "10.1175/2007JCLI2065.1",
        "issn": "0894-8755",
        "publisher": "American Meteorological Society",
        "publication": "Journal of Climate",
        "publication_date": "2008-08-01",
        "series_number": "15",
        "volume": "21",
        "issue": "15",
        "pages": "3815-3832"
    },
    {
        "id": "authors:q4dc0-94k73",
        "collection": "authors",
        "collection_id": "q4dc0-94k73",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:BORng08",
        "type": "article",
        "title": "Monsoons as eddy-mediated regime transitions of the tropical overturning circulation",
        "author": [
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Monsoons are generally viewed as planetary-scale sea-breeze circulations, caused by contrasts in the thermal properties between oceans and land surfaces that lead to thermal contrasts upon radiative heating1, 2. But the radiative heating evolves gradually with the seasons, whereas the onset of monsoon precipitation, and the associated circulation changes such as reversal of surface winds, occur rapidly3, 4. Here we use reanalysis data to show that the onset of the Asian monsoon marks a transition between two circulation regimes that are distinct in the degree to which eddy momentum fluxes control the strength of the tropical overturning circulation. Rapid transitions of the circulation between the two regimes can occur as a result of feedbacks between large-scale extratropical eddies and the tropical circulation5. Using simulations with an aquaplanet general circulation model, we demonstrate that rapid, eddy-mediated monsoon transitions occur even in the absence of surface inhomogeneities, provided the planet surface has sufficiently low thermal inertia. On the basis of these results, we propose a view of monsoons in which feedbacks between large-scale extratropical eddies and the tropical circulation are essential for the development of monsoons, whereas surface inhomogeneities such as land-sea contrasts are not.",
        "doi": "10.1038/ngeo248",
        "issn": "1752-0894",
        "publisher": "Nature Publishing Group",
        "publication": "Nature Geoscience",
        "publication_date": "2008-08",
        "series_number": "8",
        "volume": "1",
        "issue": "8",
        "pages": "515-519"
    },
    {
        "id": "authors:bjzqg-cry21",
        "collection": "authors",
        "collection_id": "bjzqg-cry21",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas08b",
        "type": "article",
        "title": "Scaling Laws and Regime Transitions of Macroturbulence in Dry Atmospheres",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Walker",
                "given_name": "Christopher C.",
                "clpid": "Walker-C-C"
            }
        ],
        "abstract": "In simulations of a wide range of circulations with an idealized general circulation model, clear scaling laws of dry atmospheric macroturbulence emerge that are consistent with nonlinear eddy\u2013eddy interactions being weak. The simulations span several decades of eddy energies and include Earth-like circulations and circulations with multiple jets and belts of surface westerlies in each hemisphere. In the simulations, the eddy available potential energy and the barotropic and baroclinic eddy kinetic energy scale linearly with each other, with the ratio of the baroclinic eddy kinetic energy to the barotropic eddy kinetic energy and eddy available potential energy decreasing with increasing planetary radius and rotation rate. Mean values of the meridional eddy flux of surface potential temperature and of the vertically integrated convergence of the meridional eddy flux of zonal momentum generally scale with functions of the eddy energies and the energy-containing eddy length scale, with a few exceptions in simulations with statically near-neutral or neutral extratropical thermal stratifications. Eddy energies scale with the mean available potential energy and with a function of the supercriticality, a measure of the near-surface slope of isentropes. Strongly baroclinic circulations form an extended regime in which eddy energies scale linearly with the mean available potential energy. Mean values of the eddy flux of surface potential temperature and of the vertically integrated eddy momentum flux convergence scale similarly with the mean available potential energy and other mean fields. \n\nThe scaling laws for the dependence of eddy fields on mean fields exhibit a regime transition between a regime in which the extratropical thermal stratification and tropopause height are controlled by radiation and convection and a regime in which baroclinic entropy fluxes modify the extratropical thermal stratification and tropopause height. At the regime transition, for example, the dependence of the eddy flux of surface potential temperature and the dependence of the vertically integrated eddy momentum flux convergence on mean fields changes -\u2014 a result with implications for climate stability and for the general circulation of an atmosphere, including its tropical Hadley circulation.",
        "doi": "10.1175/2007JAS2616.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2008-07",
        "series_number": "7",
        "volume": "65",
        "issue": "7",
        "pages": "2153-5173"
    },
    {
        "id": "authors:41gsj-1pt46",
        "collection": "authors",
        "collection_id": "41gsj-1pt46",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:MARjas08",
        "type": "article",
        "title": "Statistics of an Unstable Barotropic Jet from a Cumulant Expansion",
        "author": [
            {
                "family_name": "Marston",
                "given_name": "J. B.",
                "clpid": "Marston-J-B"
            },
            {
                "family_name": "Conover",
                "given_name": "E.",
                "clpid": "Conover-E"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Low-order equal-time statistics of a barotropic flow on a rotating sphere are investigated. The flow is driven by linear relaxation toward an unstable zonal jet. For relatively short relaxation times, the flow is dominated by critical-layer waves. For sufficiently long relaxation times, the flow is turbulent. Statistics obtained from a second-order cumulant expansion are compared to those accumulated in direct numerical simulations, revealing the strengths and limitations of the expansion for different relaxation times.",
        "doi": "10.1175/2007JAS2510.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2008-06",
        "series_number": "6",
        "volume": "65",
        "issue": "6",
        "pages": "1955-1966"
    },
    {
        "id": "authors:kj7ky-7h698",
        "collection": "authors",
        "collection_id": "kj7ky-7h698",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas08a",
        "type": "article",
        "title": "Eddy-Mediated Regime Transitions in the Seasonal Cycle of a Hadley Circulation and Implications for Monsoon Dynamics",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Bordoni",
                "given_name": "Simona",
                "orcid": "0000-0003-4771-3350",
                "clpid": "Bordoni-S"
            }
        ],
        "abstract": "In a simulation of seasonal cycles with an idealized general circulation model without a hydrologic cycle and with zonally symmetric boundary conditions, the Hadley cells undergo transitions between two regimes distinguishable according to whether large-scale eddy momentum fluxes strongly or weakly influence the strength of a cell. The center of the summer and equinox Hadley cell lies in a latitude zone of upper-level westerlies and significant eddy momentum flux divergence; the influence of eddy momentum fluxes on the strength of the cell is strong. The center of the cross-equatorial winter Hadley cell lies in a latitude zone of upper-level easterlies and is shielded from the energy-containing midlatitude eddies; the influence of eddy momentum fluxes on the strength of the cell is weak. Mediated by feedbacks between eddy fluxes, mean zonal winds at upper levels, and the mean meridional circulation, the dominant balance in the zonal momentum equation at the center of a Hadley cell shifts at the transitions between the regimes, from eddies dominating the momentum flux divergence in the summer and equinox cell to the mean meridional circulation dominating in the winter cell. At the transitions, a feedback involving changes in the strength of the lower-level temperature advection and in the latitude of the boundary between the winter and summer cell is responsible for changes in the strength of the cross-equatorial winter cell. The transitions resemble the onset and end of monsoons, for example, in the shift in the dominant zonal momentum balance, rapid shifts in the latitudes of maximum meridional mass flux and of maximum convergence at lower levels, rapid changes in strength of the upward mass flux, and changes in direction and strength of the zonal wind at upper and lower levels. In the monsoonal regime, the maximum upward mass flux occurs in an off-equatorial convergence zone located where the balance of the meridional geopotential gradient in the planetary boundary layer shifts from nonlinear frictional to geostrophic. Similar dynamic mechanisms as at the regime transitions in the simulation\u2014mechanisms that can act irrespective of land\u2013sea contrasts and other inhomogeneities in lower boundary conditions\u2014may be implicated in large-scale monsoon dynamics in Earth's atmosphere.",
        "doi": "10.1175/2007JAS2415.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2008-03",
        "series_number": "3",
        "volume": "65",
        "issue": "3",
        "pages": "915-934"
    },
    {
        "id": "authors:knsmy-3aw78",
        "collection": "authors",
        "collection_id": "knsmy-3aw78",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:OGOjas08",
        "type": "article",
        "title": "Weather-Layer Dynamics of Baroclinic Eddies and Multiple Jets in an Idealized General Circulation Model",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The general circulation and the behavior of multiple jets and baroclinic eddies are described for an atmosphere in which meridional potential temperature gradients and eddies are confined to a weather layer. The weather layer is separated from the frictional lower boundary by a statically stable barotropic layer with significant mass. Closure of the zonal momentum budget in the resulting circulation is achieved through ageostrophic meridional cells that extend to the lower boundary, at which momentum is dissipated. In a series of simulations with a multilevel primitive equation model, dynamic changes in the static stability of the weather layer are found to be critical in determining the scaling of the baroclinic eddies, an effect not captured in quasigeostrophic models. For simulations with a single jet in each hemisphere, the static stability of the weather layer adjusts so that a significant inverse energy cascade to scales larger than the Rossby deformation radius does not occur. The eddy length is found to scale with both the Rossby deformation radius and the Rhines scale. Simulations with larger planetary radii and low pole-to-equator temperature gradients exhibit multiple jets in each hemisphere. Eddy lengths and energies for the jet nearest the equator in each hemisphere have the same scaling as those in the single-jet simulations. Similar scalings are found for jets farther poleward but with different constants of proportionality that are consistent with more supercritical eddies. The local eddy length is found to have only a weak variation with latitude, and the local meridional jet spacing is found to scale with the local eddy length in all cases. Insights from the weather-layer simulations may be relevant to circulations in gas giant planets and the ocean.",
        "doi": "10.1175/2007JAS2280.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2008-02",
        "series_number": "2",
        "volume": "65",
        "issue": "2",
        "pages": "524-535"
    },
    {
        "id": "authors:rqtq2-0y045",
        "collection": "authors",
        "collection_id": "rqtq2-0y045",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:KORjc07",
        "type": "article",
        "title": "A Climatology of the Tropospheric Thermal Stratification Using Saturation Potential Vorticity",
        "author": [
            {
                "family_name": "Korty",
                "given_name": "Robert L.",
                "clpid": "Korty-R-L"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The condition of convective neutrality is assessed in the troposphere by calculating the saturation potential vorticity P* from reanalysis data. Regions of the atmosphere in which saturation entropy is constant along isosurfaces of absolute angular momentum, a state indicative of slantwise-convective neutrality, have values of P* equal to zero. In a global reanalysis dataset spanning the years 1970\u20132004, tropospheric regions are identified in which P* is near zero, implying that vertical convection or slantwise convection may be important in determining the local thermal stratification. Convectively neutral air masses are common not only in the Tropics but also in higher latitudes, for example, over midlatitude continents in summer and in storm tracks over oceans in winter. Large-scale eddies appear to stabilize parts of the lower troposphere, particularly in winter.",
        "doi": "10.1175/2007JCLI1788.1",
        "issn": "0894-8755",
        "publisher": "Journal of Climate",
        "publication": "Journal of Climate",
        "publication_date": "2007-12-15",
        "series_number": "24",
        "volume": "20",
        "issue": "24",
        "pages": "5977-5991"
    },
    {
        "id": "authors:tqptz-34f72",
        "collection": "authors",
        "collection_id": "tqptz-34f72",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-154729045",
        "type": "article",
        "title": "Recovery of atmospheric flow statistics in a general circulation model without nonlinear eddy-eddy interactions",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The closure problem of turbulence arises because nonlinear interactions among turbulent fluctuations (eddies) lead to an infinite hierarchy of moment equations for flow statistics. Here we demonstrate with an idealized general circulation model (GCM) that many atmospheric flow statistics can already be recovered if the hierarchy of moment equations is truncated at second order, corresponding to the elimination of nonlinear eddy-eddy interactions. Some, but not all, features of the general circulation remain the same. The atmospheric eddy kinetic energy spectrum retains a \u22123 power-law range even though this is usually explained in terms of an enstrophy cascade mediated by nonlinear eddy-eddy interactions. Our results suggest that it may be possible to construct fast general circulation models that solve for atmospheric flow statistics directly rather than via simulation of individual eddies and their interactions.",
        "doi": "10.1029/2007GL031779",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2007-11",
        "series_number": "22",
        "volume": "34",
        "issue": "22",
        "pages": "Art. No. L22801"
    },
    {
        "id": "authors:ava4q-yqw78",
        "collection": "authors",
        "collection_id": "ava4q-yqw78",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20150317-075915988",
        "type": "article",
        "title": "Uncertainty in climate-sensitivity estimates",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Based on reconstructions of past temperatures from proxy data, Hegerl et al. estimate a confidence interval for climate sensitivity that suggests a substantially reduced probability of very high climate sensitivity compared with previous empirical estimates. Here I show that the inference procedure used by Hegerl et al. neglects uncertainties in temperature reconstructions and in the estimated climate sensitivity and can even be used to infer that the climate sensitivity is zero with vanishing uncertainty. Similar procedures based on temperature reconstructions from proxy data generally underestimate uncertainties in climate sensitivity.",
        "doi": "10.1038/nature05707",
        "issn": "0028-0836",
        "publisher": "Nature Publishing Group",
        "publication": "Nature",
        "publication_date": "2007-03-01",
        "series_number": "7131",
        "volume": "446",
        "issue": "7131",
        "pages": "E1"
    },
    {
        "id": "authors:8e7gx-ygj54",
        "collection": "authors",
        "collection_id": "8e7gx-ygj54",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNnpg07",
        "type": "article",
        "title": "Comment on \"Spatio-temporal filling of missing points in geophysical data sets\" by D. Kondrashov and M. Ghil, Nonlin. Processes Geophys., 13, 151\u2013159, 2006",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "T.",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Kondrashov and Ghil (2006) (KG hereafter) describe a method for imputing missing values in incomplete datasets that can exploit both spatial and temporal covariability to estimate missing values from available values. Temporal covariability has not been exploited as widely as spatial covariability in imputing missing values in geophysical datasets, but, as KG show, doing so can improve estimates of missing values. However, there are several inaccuracies in KG's paper. Since similar inaccuracies have surfaced in other recent papers, for example, in the literature on paleo-climate reconstructions, I would like to point them out here.",
        "doi": "10.5194/npg-14-1-2007",
        "issn": "1023-5809",
        "publisher": "European Geosciences Union",
        "publication": "Nonlinear Processes in Geophysics",
        "publication_date": "2007-01-15",
        "series_number": "1",
        "volume": "14",
        "issue": "1",
        "pages": "1-2"
    },
    {
        "id": "authors:4bcvk-fc148",
        "collection": "authors",
        "collection_id": "4bcvk-fc148",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:WALjas06",
        "type": "article",
        "title": "Eddy Influences on Hadley Circulations: Simulations with an Idealized GCM",
        "author": [
            {
                "family_name": "Walker",
                "given_name": "Christopher C.",
                "clpid": "Walker-C-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "An idealized GCM is used to investigate how the strength and meridional extent of the Hadley circulation depend on the planet radius, rotation rate, and thermal driving. Over wide parameter ranges, the strength and meridional extent of the Hadley circulation display clear scaling relations with regime transitions, which are not predicted by existing theories of axisymmetric Hadley circulations. For example, the scaling of the strength as a function of the radiative-equilibrium equator-to-pole temperature contrast exhibits a regime transition corresponding to a regime transition in scaling laws of baroclinic eddy fluxes. The scaling of the strength of the cross-equatorial Hadley cell as a function of the latitude of maximum radiative-equilibrium temperature exhibits a regime transition from a regime in which eddy momentum fluxes strongly influence the strength to a regime in which the influence of eddy momentum fluxes is weak. \n\nOver a wide range of flow parameters, albeit not always, the Hadley circulation strength is directly related to the eddy momentum flux divergence at the latitude of the streamfunction extremum. Simulations with hemispherically symmetric thermal driving span circulations with local Rossby numbers in the horizontal upper branch of the Hadley circulation between 0.1 and 0.8, indicating that neither nonlinear nearly inviscid theories, valid for Ro \u2192 1, nor linear theories, valid for Ro \u2192 0, of axisymmetric Hadley circulations can be expected to be generally adequate. Nonlinear theories of axisymmetric Hadley circulations may account for aspects of the circulation when the maximum radiative-equilibrium temperature is displaced sufficiently far away from the equator, which results in cross-equatorial Hadley cells with nearly angular momentum-conserving upper branches. \n\nThe dependence of the Hadley circulation on eddy fluxes, which are themselves dependent on extratropical circulation characteristics such as meridional temperature gradients, suggests that tropical circulations depend on the extratropical climate.",
        "doi": "10.1175/JAS3821.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2006-12",
        "series_number": "12",
        "volume": "63",
        "issue": "12",
        "pages": "3333-3360"
    },
    {
        "id": "authors:wg56b-4pa74",
        "collection": "authors",
        "collection_id": "wg56b-4pa74",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjc06",
        "type": "article",
        "title": "A Climatology of Tropospheric Zonal-Mean Water Vapor Fields and Fluxes in Isentropic Coordinates",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Smith",
                "given_name": "Karen L.",
                "orcid": "0000-0001-5785-7038",
                "clpid": "Smith-K-L"
            },
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Walker",
                "given_name": "Christopher C.",
                "clpid": "Walker-C-C"
            }
        ],
        "abstract": "Based on reanalysis data for the years 1980\u20132001 from the European Centre for Medium-Range Weather Forecasts (ERA-40 data), a climatology of tropospheric zonal-mean water vapor fields and fluxes in isentropic coordinates is presented. In the extratropical free troposphere, eddy fluxes dominate the meridional flux of specific humidity along isentropes. At all levels, isentropic eddy fluxes transport water vapor from the deep Tropics through the subtropics into the extratropics. Isentropic eddy fluxes of specific humidity diverge near the surface and in the tropical and subtropical free troposphere; they converge in the extratropical free troposphere. Isentropic mean advective fluxes of specific humidity play a secondary role in the meridional water vapor transport in the free troposphere; however, they dominate the meridional flux of specific humidity near the surface, where they transport water vapor equatorward and, in the solstice seasons, across the equator. Cross-isentropic mean advective fluxes of specific humidity are especially important in the Hadley circulation, in whose ascending branches they moisten and in whose descending branches they dry the free troposphere. \n\nNear the minima of zonal-mean relative humidity in the subtropical free troposphere, the divergence of the cross-isentropic mean advective flux of specific humidity in the descending branches of the Hadley circulation is the dominant divergence in the mean specific humidity balance; it is primarily balanced by convergence of cross-isentropic turbulent fluxes that transport water vapor from the surface upward. Although there are significant isentropic eddy fluxes of specific humidity through the region of the subtropical relative humidity minima, their divergence near the minima is generally small compared with the divergence of cross-isentropic mean advective fluxes, implying that moistening by eddy transport from the Tropics into the region of the minima approximately balances drying by eddy transport into the extratropics. That drying by cross-isentropic mean subsidence near the subtropical relative humidity minima is primarily balanced by moistening by upward turbulent fluxes of specific humidity, likely in convective clouds, suggests cloud dynamics may play a central role in controlling the relative humidity of the subtropical free troposphere.",
        "doi": "10.1175/JCLI3931.1",
        "issn": "0894-8755",
        "publisher": "Journal of Climate",
        "publication": "Journal of Climate",
        "publication_date": "2006-11-15",
        "series_number": "22",
        "volume": "19",
        "issue": "22",
        "pages": "5918-5933"
    },
    {
        "id": "authors:4gxxj-bb603",
        "collection": "authors",
        "collection_id": "4gxxj-bb603",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:OGOjas06",
        "type": "article",
        "title": "Stochastic Models for the Kinematics of Moisture Transport and Condensation in Homogeneous Turbulent Flows",
        "author": [
            {
                "family_name": "O'Gorman",
                "given_name": "Paul A.",
                "clpid": "O'Gorman-P-A"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The transport of a condensing passive scalar is studied as a prototype model for the kinematics of moisture transport on isentropic surfaces. Condensation occurs whenever the scalar concentration exceeds a specified local saturation value. Since condensation rates are strongly nonlinear functions of moisture content, the mean moisture flux is generally not diffusive. To relate the mean moisture content, mean condensation rate, and mean moisture flux to statistics of the advecting velocity field, a one-dimensional stochastic model is developed in which the Lagrangian velocities of air parcels are independent Ornstein\u2013Uhlenbeck (Gaussian colored noise) processes. The mean moisture evolution equation for the stochastic model is derived in the Brownian and ballistic limits of small and large Lagrangian velocity correlation time. The evolution equation involves expressions for the mean moisture flux and mean condensation rate that are nonlocal but remarkably simple. In a series of simulations of homogeneous two-dimensional turbulence, the dependence of mean moisture flux and mean condensation rate on mean saturation deficit is shown to be reproducible by the one-dimensional stochastic model, provided eddy length and time scales are taken as given. For nonzero Lagrangian velocity correlation times, condensation reduces the mean moisture flux for a given mean moisture gradient compared with the mean flux of a noncondensing scalar.",
        "doi": "10.1175/JAS3794.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2006-11",
        "series_number": "11",
        "volume": "63",
        "issue": "11",
        "pages": "2992-3005"
    },
    {
        "id": "authors:md7mh-r2f20",
        "collection": "authors",
        "collection_id": "md7mh-r2f20",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas06",
        "type": "article",
        "title": "Self-Organization of Atmospheric Macroturbulence into Critical States of Weak Nonlinear Eddy\u2013Eddy Interactions",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Walker",
                "given_name": "Christopher C.",
                "clpid": "Walker-C-C"
            }
        ],
        "abstract": "It is generally held that atmospheric macroturbulence can be strongly nonlinear. Yet weakly nonlinear models successfully account for scales and structures of baroclinic eddies in Earth's atmosphere. Here a theory and simulations with an idealized GCM are presented that suggest weakly nonlinear models are so successful because atmospheric macroturbulence organizes itself into critical states of weak nonlinear eddy\u2013eddy interactions. By modifying the thermal structure of the extratropical atmosphere such that its supercriticality remains limited, macroturbulence inhibits nonlinear eddy\u2013eddy interactions and the concomitant inverse energy cascade from the length scales of baroclinic instability to larger scales. For small meridional surface temperature gradients, the extratropical thermal stratification and tropopause height are set by radiation and convection, and the supercriticality is less than one; for sufficiently large meridional surface temperature gradients, the extratropical thermal stratification and tropopause height are modified by baroclinic eddies such that the supercriticality does not significantly exceed one. In either case, the scale of the energy-containing eddies is similar to the scale of the linearly most unstable baroclinic waves, and eddy kinetic and available potential energies are equipartitioned. The theory and simulations point to fundamental constraints on the thermal structures and global circulations of the atmospheres of Earth and other planets, for example, by providing limits on the tropopause height and estimates for eddy scales, eddy energies, and jet separation scales.",
        "doi": "10.1175/JAS3699.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2006-06",
        "series_number": "6",
        "volume": "63",
        "issue": "6",
        "pages": "1569-1586"
    },
    {
        "id": "authors:x4160-zdv26",
        "collection": "authors",
        "collection_id": "x4160-zdv26",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNbams06b",
        "type": "article",
        "title": "Global Circulation of the Atmosphere (2004)",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Sobel",
                "given_name": "Adam",
                "clpid": "Sobel-A"
            }
        ],
        "abstract": "GLOBAL CIRCULATION OF THE ATMOSPHERE\nWHAT: Experts assembled to assess understanding of the global circulation with an eye toward identifying outstanding questions and improving the framework for synthesizing observations and simulations.\nWHEN: 4\u20136 November 2004\nWHERE: Pasadena, California",
        "doi": "10.1175/BAMS-87-6-807",
        "issn": "0003-0007",
        "publisher": "Bulletin of the American Meteorological Society",
        "publication": "Bulletin of the American Meteorological Society",
        "publication_date": "2006-06",
        "series_number": "6",
        "volume": "87",
        "issue": "6",
        "pages": "807-809"
    },
    {
        "id": "authors:0b9y8-x2e37",
        "collection": "authors",
        "collection_id": "0b9y8-x2e37",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNareps06",
        "type": "article",
        "title": "The general circulation of the atmosphere",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Theories of how Earth's surface climate may change in the future, of how it may have been in the past, and of how it is related to climates of other planets must build upon a theory of the general circulation of the atmosphere. The view of the atmospheric general circulation presented here focuses not on Earth's general circulation as such but on a continuum of idealized circulations with axisymmetric flow statistics. Analyses of observational data for Earth's atmosphere, simulations with idealized general circulation models, and theoretical considerations suggest how characteristics of the tropical Hadley circulation, of the extratropical circulation, and of atmospheric macroturbulence may depend on parameters such as the planet radius and rotation rate and the strength of the differential heating at the surface.",
        "doi": "10.1146/annurev.earth.34.031405.125144",
        "issn": "0084-6597",
        "publisher": "Annual Reviews",
        "publication": "Annual Review of Earth and Planetary Sciences",
        "publication_date": "2006-05",
        "volume": "34",
        "pages": "655-688"
    },
    {
        "id": "authors:q7rtv-yjd06",
        "collection": "authors",
        "collection_id": "q7rtv-yjd06",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas05",
        "type": "article",
        "title": "Zonal momentum balance, potential vorticity dynamics, and mass fluxes on near-surface isentropes",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "While it has been recognized for some time that isentropic coordinates provide a convenient framework for theories of the global circulation of the atmosphere, the role of boundary effects in the zonal momentum balance and in potential vorticity dynamics on isentropes that intersect the surface has remained unclear. Here, a balance equation is derived that describes the temporal and zonal mean balance of zonal momentum and of potential vorticity on isentropes, including the near-surface isentropes that sometimes intersect the surface. Integrated vertically, the mean zonal momentum or potential vorticity balance leads to a balance condition that relates the mean meridional mass flux along isentropes to eddy fluxes of potential vorticity and surface potential temperature. The isentropic-coordinate balance condition formally resembles balance conditions well known in quasigeostrophic theory, but on near-surface isentropes it generally differs from the quasigeostrophic balance conditions. Not taking the intersection of isentropes with the surface into account, quasigeostrophic theory does not adequately represent the potential vorticity dynamics and mass fluxes on near-surface isentropes\u2014a shortcoming that calls into question the relevance of quasigeostrophic theories for the macroturbulence and global circulation of the atmosphere.",
        "doi": "10.1175/JAS3341.1",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2005-06",
        "series_number": "6",
        "volume": "62",
        "issue": "6",
        "pages": "1884-1900"
    },
    {
        "id": "authors:d3x1g-a1892",
        "collection": "authors",
        "collection_id": "d3x1g-a1892",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-110409542",
        "type": "article",
        "title": "Response of idealized Hadley circulations to seasonally varying heating",
        "author": [
            {
                "family_name": "Walker",
                "given_name": "Chris C.",
                "clpid": "Walker-C-C"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "[1] The response of Hadley circulations to displacements of the latitude of maximum heating is investigated in idealized axisymmetric and eddy-permitting models. Consistent with an earlier study and with theory for the nearly inviscid limit (Lindzen and Hou, 1988), the strength of the Hadley circulation is sensitive to displacements of heating: the winter cell strengthens and summer cell weakens when the maximum heating is displaced off the equator. However, in conflict with the nearly inviscid limit but consistent with observations of Earth's atmosphere, the strength of an annually averaged Hadley circulation is comparable to the Hadley circulation driven by an annually averaged heating. The disagreement between these results and the nearly inviscid limit is ascribed to vertical diffusion of momentum and dry static energy in the axisymmetric model and to baroclinic eddy fluxes in the eddy-permitting model. Nonlinear amplification of the annually averaged Hadley circulation is only seen near the upper boundary in simulations with a rigid lid near the tropopause, suggesting that the amplification is an artifact of the upper boundary condition.",
        "doi": "10.1029/2004GL022304",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2005-03",
        "series_number": "6",
        "volume": "32",
        "issue": "6",
        "pages": "Art. No. L06813"
    },
    {
        "id": "authors:sp2dq-bqk83",
        "collection": "authors",
        "collection_id": "sp2dq-bqk83",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-104900408",
        "type": "article",
        "title": "Using generalized cross-validation to select parameters in inversions for regional carbon fluxes",
        "author": [
            {
                "family_name": "Krakauer",
                "given_name": "Nir Y.",
                "clpid": "Krakauer-N-Y"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Randerson",
                "given_name": "James T.",
                "orcid": "0000-0001-6559-7387",
                "clpid": "Randerson-J-T"
            },
            {
                "family_name": "Olsen",
                "given_name": "Seth C.",
                "clpid": "Olsen-S-C"
            }
        ],
        "abstract": "[1] Estimating CO_2 fluxes from the pattern of atmospheric CO_2 concentrations with atmospheric transport models is an ill-posed inverse problem, whose solution is stabilized using prior information. Weights assigned to prior information and to CO_2 concentrations at different locations are quantified by parameters that are not well known, and differences in the choice of these parameters contribute to differences among published estimates of the regional partitioning of CO_2 fluxes. Following the TransCom 3 protocol to estimate CO_2 fluxes for 1992\u20131996, we find that the partitioning of the CO_2 sink between land and oceans and between North America and Eurasia depends on parameters that quantify the relative weight given to prior flux estimates and the extent to which CO_2 concentrations at different stations are differentially weighted. Parameter values that minimize an estimated prediction error can be chosen by generalized cross-validation (GCV). The GCV parameter values yield fluxes in northern regions similar to those obtained with the TransCom parameter values, but the GCV fluxes are smaller in the poorly constrained equatorial and southern regions.",
        "doi": "10.1029/2004GL020323",
        "issn": "0094-8276",
        "publisher": "American Geophysical Union",
        "publication": "Geophysical Research Letters",
        "publication_date": "2004-10",
        "series_number": "19",
        "volume": "31",
        "issue": "19",
        "pages": "Art. No. L19108"
    },
    {
        "id": "authors:cv4qq-jd814",
        "collection": "authors",
        "collection_id": "cv4qq-jd814",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas04",
        "type": "article",
        "title": "The tropopause and the thermal stratification in the extratropics of a dry atmosphere",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "A dynamical constraint on the extratropical tropopause height and thermal stratification is derived by considerations of entropy fluxes, or isentropic mass fluxes, and their different magnitudes in the troposphere and stratosphere. The dynamical constraint is based on a relation between isentropic mass fluxes and eddy fluxes of potential vorticity and surface potential temperature and on diffusive eddy flux closures. It takes baroclinic eddy fluxes as central for determining the extratropical tropopause height and thermal stratification and relates the tropopause potential temperature approximately linearly to the surface potential temperature and its gradient.\n\nSimulations with an idealized GCM point to the possibility of an extratropical climate in which baroclinic eddy fluxes maintain a statically stable thermal stratification and, in interaction with large-scale diabatic processes, lead to the formation of a sharp tropopause. The simulations show that the extratropical tropopause height and thermal stratification are set locally by extratropical processes and do not depend on tropical processes and that, across a wide range of atmospheric circulations, the dynamical constraint describes the relation between tropopause and surface potential temperatures well. An analysis of observational data shows that the dynamical constraint, derived for an idealized dry atmosphere, can account for interannual variations of the tropopause height and thermal stratification in the extratropics of the earth's atmosphere.\n\nThe dynamical constraint implies that if baroclinic eddies determine the tropopause height and thermal stratification, an atmosphere organizes itself into a state in which nonlinear interactions among eddies are inhibited. The inhibition of nonlinear eddy\u2013eddy interactions offers an explanation for the historic successes of linear and weakly nonlinear models of large-scale extratropical dynamics.",
        "doi": "10.1175/1520-0469(2004)061<1317:TTATTS>2.0.CO;2",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2004-06-15",
        "series_number": "12",
        "volume": "61",
        "issue": "12",
        "pages": "1317-1340"
    },
    {
        "id": "authors:2v724-0qk07",
        "collection": "authors",
        "collection_id": "2v724-0qk07",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjas03",
        "type": "article",
        "title": "Boundary effects in potential vorticity dynamics",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Held",
                "given_name": "Isaac M.",
                "clpid": "Held-I-M"
            },
            {
                "family_name": "Garner",
                "given_name": "Stephen T.",
                "clpid": "Garner-S-T"
            }
        ],
        "abstract": "Many aspects of geophysical flows can be described compactly in terms of potential vorticity dynamics. Since potential temperature can fluctuate at boundaries, however, the boundary conditions for potential vorticity dynamics are inhomogeneous, which complicates considerations of potential vorticity dynamics when boundary effects are dynamically significant. \n\nA formulation of potential vorticity dynamics is presented that encompasses boundary effects. It is shown that, for arbitrary flows, the generalization of the potential vorticity concept to a sum of the conventional interior potential vorticity and a singular surface potential vorticity allows one to replace the inhomogeneous boundary conditions for potential vorticity dynamics by simpler homogeneous boundary conditions (of constant potential temperature). Functional forms of the surface potential vorticity are derived from field equations in which the potential vorticity and a potential vorticity flux appear as sources of flow quantities in the same way in which an electric charge and an electric current appear as sources of fields in electrodynamics. For the generalized potential vorticity of flows that need be neither balanced nor hydrostatic and that can be influenced by diabatic processes and friction, a conservation law holds that is similar to the conservation law for the conventional interior potential vorticity. The conservation law for generalized potential vorticity contains, in the quasigeostrophic limit, the well-known dual relationship between fluctuations of potential temperature at boundaries and fluctuations of potential vorticity in the interior of quasigeostrophic flows. A nongeostrophic effect described by the conservation law is the induction of generalized potential vorticity by baroclinicity at boundaries, an effect that plays a role, for example, in mesoscale flows past topographic obstacles. Based on the generalized potential vorticity concept, a theory is outlined of how a wake with lee vortices can form in weakly dissipative flows past a mountain. Theoretical considerations and an analysis of a simulation show that a wake with lee vortices can form by separation of a generalized potential vorticity sheet from the mountain surface, similar to the separation of a friction-induced vorticity sheet from an obstacle, except that the generalized potential vorticity sheet can be induced by baroclinicity at the surface.",
        "doi": "10.1175/1520-0469(2003)60<1024:BEIPVD>2.0.CO;2",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "2003-04-15",
        "series_number": "8",
        "volume": "60",
        "issue": "8",
        "pages": "1024-1040"
    },
    {
        "id": "authors:5e18h-2w622",
        "collection": "authors",
        "collection_id": "5e18h-2w622",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjc01b",
        "type": "article",
        "title": "Analysis of Incomplete Climate Data: Estimation of Mean Values and Covariance Matrices and Imputation of Missing Values",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "Estimating the mean and the covariance matrix of an incomplete dataset and filling in missing values with imputed values is generally a nonlinear problem, which must be solved iteratively. The expectation maximization (EM) algorithm for Gaussian data, an iterative method both for the estimation of mean values and covariance matrices from incomplete datasets and for the imputation of missing values, is taken as the point of departure for the development of a regularized EM algorithm. In contrast to the conventional EM algorithm, the regularized EM algorithm is applicable to sets of climate data, in which the number of variables typically exceeds the sample size. The regularized EM algorithm is based on iterated analyses of linear regressions of variables with missing values on variables with available values, with regression coefficients estimated by ridge regression, a regularized regression method in which a continuous regularization parameter controls the filtering of the noise in the data. The regularization parameter is determined by generalized cross-validation, such as to minimize, approximately, the expected mean-squared error of the imputed values. The regularized EM algorithm can estimate, and exploit for the imputation of missing values, both synchronic and diachronic covariance matrices, which may contain information on spatial covariability, stationary temporal covariability, or cyclostationary temporal covariability. A test of the regularized EM algorithm with simulated surface temperature data demonstrates that the algorithm is applicable to typical sets of climate data and that it leads to more accurate estimates of the missing values than a conventional noniterative imputation technique.",
        "doi": "10.1175/1520-0442(2001)014<0853:AOICDE>2.0.CO;2",
        "issn": "0894-8755",
        "publisher": "Journal of Climate",
        "publication": "Journal of Climate",
        "publication_date": "2001-03-01",
        "series_number": "5",
        "volume": "14",
        "issue": "5",
        "pages": "853-871"
    },
    {
        "id": "authors:dkm0v-bgs32",
        "collection": "authors",
        "collection_id": "dkm0v-bgs32",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:20160930-153541748",
        "type": "article",
        "title": "Algorithm 808: ARfit\u2014a Matlab package for the estimation of parameters and eigenmodes of multivariate autoregressive models",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Neumaier",
                "given_name": "Arnold",
                "clpid": "Neumaier-A"
            }
        ],
        "abstract": "ARfit is a collection of Matlab modules for modeling and analyzing multivariate time series with autoregressive (AR) models. ARfit contains modules to given time series data, for analyzing eigen modes of a fitted model, and for simulating AR processes. ARfit estimates the parameters of AR models from given time series data with a stepwise least squares algorithm that is computationally efficient, in particular when the data are high-dimensional. ARfit modules construct approximate confidence intervals for the estimated parameters and compute statistics with which the adequacy of a fitted model can be assessed. Dynamical characteristics of the modeled time series can be examined by means of a decomposition of a fitted AR model into eigenmodes and associated oscillation periods, damping times, and excitations. The ARfit module that performs the eigendecomposition of a fitted model also constructs approximate confidence intervals for the eigenmodes and their oscillation periods and damping times.",
        "doi": "10.1145/382043.382316",
        "issn": "0098-3500",
        "publisher": "ACM",
        "publication": "ACM Transactions on Mathematical Software (TOMS)",
        "publication_date": "2001-03",
        "series_number": "1",
        "volume": "27",
        "issue": "1",
        "pages": "58-65"
    },
    {
        "id": "authors:ezy8h-pmd03",
        "collection": "authors",
        "collection_id": "ezy8h-pmd03",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHN01a",
        "type": "article",
        "title": "Discriminants of Twentieth-Century Changes in Earth Surface Temperatures",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Held",
                "given_name": "Isaac M.",
                "clpid": "Held-I-M"
            }
        ],
        "abstract": "An approach to identifying climate changes is presented that does not hinge on simulations of natural climate variations or anthropogenic changes. Observed interdecadal climate variations are decomposed into several discriminants, mutually uncorrelated spatiotemporal components with a maximal ratio of interdecadal-to-intradecadal variance. The dominant discriminants of twentieth-century variations in surface temperature exhibit large-scale warming in which, particularly in the Northern Hemisphere summer months, localized cooling is embedded. The structure of the large-scale warming is consistent with expected effects of increases in greenhouse gas concentrations. The localized cooling, with maxima on scales of 1000\u20132000 km over East Asia, eastern Europe, and North America, is suggestive of radiative effects of anthropogenic sulfate aerosols.",
        "doi": "10.1175/1520-0442(2001)014<0249:LDOTCC>2.0.CO;2",
        "issn": "0894-8755",
        "publisher": "Journal of Climate",
        "publication": "Journal of Climate",
        "publication_date": "2001-02-01",
        "series_number": "3",
        "volume": "14",
        "issue": "3",
        "pages": "249-254"
    },
    {
        "id": "authors:ka1rt-fss76",
        "collection": "authors",
        "collection_id": "ka1rt-fss76",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:HELjas99",
        "type": "article",
        "title": "The Surface Branch of the Zonally Averaged Mass Transport Circulation in the Troposphere",
        "author": [
            {
                "family_name": "Held",
                "given_name": "Isaac M.",
                "clpid": "Held-I-M"
            },
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            }
        ],
        "abstract": "The near-surface branch of the overturning mass transport circulation in the troposphere, containing the equatorward flow, is examined in isentropic and geometric coordinates. A discussion of the zonal momentum balance within isentropic layers shows that the equatorward flow at a given latitude is confined to isentropic layers that typically intersect the surface at that latitude. As a consequence of mass transport within the surface mixed layer, much of the equatorward flow occurs in layers with potential temperatures below the mean surface potential temperature. \n\nIn the conventional transformed Eulerian mean formulation for geometric coordinates, the surface branch of the overturning circulation is represented in an unrealistic manner: streamlines of the residual circulation do not close above the surface. A modified residual circulation is introduced that is free from this defect and has the additional advantage that its computation, unlike that of the conventional residual circulation, does not require division by the static stability, which may approach zero in the planetary boundary layer. It is then argued that cold air advection by the residual circulation is responsible for the formation of surface inversions at all latitudes in idealized GCMs with weak thermal damping. Also included is a discussion of how a general circulation theory for the troposphere must be built upon a theory for the near-surface meridional mass fluxes.",
        "doi": "10.1175/1520-0469(1999)056<1688:TSBOTZ>2.0.CO;2",
        "issn": "0022-4928",
        "publisher": "American Meteorological Society",
        "publication": "Journal of the Atmospheric Sciences",
        "publication_date": "1999-11",
        "series_number": "11",
        "volume": "56",
        "issue": "11",
        "pages": "1688-1697"
    },
    {
        "id": "authors:7qrte-x5g48",
        "collection": "authors",
        "collection_id": "7qrte-x5g48",
        "cite_using_url": "https://resolver.caltech.edu/CaltechAUTHORS:SCHNjc99",
        "type": "article",
        "title": "A Conceptual Framework for Predictability Studies",
        "author": [
            {
                "family_name": "Schneider",
                "given_name": "Tapio",
                "orcid": "0000-0001-5687-2287",
                "clpid": "Schneider-T"
            },
            {
                "family_name": "Griffies",
                "given_name": "Stephen M.",
                "clpid": "Griffies-S-M"
            }
        ],
        "abstract": "A conceptual framework is presented for a unified treatment of issues arising in a variety of predictability studies. The predictive power (PP), a predictability measure based on information\u2013theoretical principles, lies at the center of this framework. The PP is invariant under linear coordinate transformations and applies to multivariate predictions irrespective of assumptions about the probability distribution of prediction errors. For univariate Gaussian predictions, the PP reduces to conventional predictability measures that are based upon the ratio of the rms error of a model prediction over the rms error of the climatological mean prediction. \n\nSince climatic variability on intraseasonal to interdecadal timescales follows an approximately Gaussian distribution, the emphasis of this paper is on multivariate Gaussian random variables. Predictable and unpredictable components of multivariate Gaussian systems can be distinguished by predictable component analysis, a procedure derived from discriminant analysis: seeking components with large PP leads to an eigenvalue problem, whose solution yields uncorrelated components that are ordered by PP from largest to smallest. \n\nIn a discussion of the application of the PP and the predictable component analysis in different types of predictability studies, studies are considered that use either ensemble integrations of numerical models or autoregressive models fitted to observed or simulated data. \n\nAn investigation of simulated multidecadal variability of the North Atlantic illustrates the proposed methodology. Reanalyzing an ensemble of integrations of the Geophysical Fluid Dynamics Laboratory coupled general circulation model confirms and refines earlier findings. With an autoregressive model fitted to a single integration of the same model, it is demonstrated that similar conclusions can be reached without resorting to computationally costly ensemble integrations.",
        "doi": "10.1175/1520-0442(1999)012<3133:ACFFPS>2.0.CO;2",
        "issn": "0894-8755",
        "publisher": "Journal of Climate",
        "publication": "Journal of Climate",
        "publication_date": "1999-10",
        "series_number": "10",
        "volume": "12",
        "issue": "10",
        "pages": "3133-3155"
    }
]