<h1>Cummings, Alan</h1>
<h2>Monograph from <a href="https://authors.library.caltech.edu">CaltechAUTHORS</a></h2>
<ul>
<li>Webber, W. R. and Lal, N., el al. (2017) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20200204-081707376">Voyager 1 Measurements Beyond the Heliopause of Galactic Cosmic Ray Helium, Boron, Carbon, Oxygen, Magnesium, Silicon and Iron Nuclei with Energies 0.5 to &gt;1.5 GeV/nuc</a>; <a href="https://doi.org/10.48550/arXiv.1712.02818">10.48550/arXiv.1712.02818</a></li>
<li>Webber, W. R. and Stone, E. C., el al. (2017) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20200204-082135453">The Intensities of Cosmic Ray H and He Nuclei at ~250 MeV/nuc Measured by Voyagers 1 and 2 - Using these Intensities to Determine the Solar Modulation Parameter in the Inner Heliosphere and the Heliosheath Over a 40 Year Time Period</a>; <a href="https://doi.org/10.48550/arXiv.1706.02772">10.48550/arXiv.1706.02772</a></li>
<li>Webber, W. R. and McDonald, F. B., el al. (2012) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20200204-084404748">At Voyager 1 Starting on about August 25, 2012 at a Distance of 121.7 AU From the Sun, a Sudden Disappearance of Anomalous Cosmic Rays and an Unusually Large Sudden Increase of Galactic Cosmic Ray H and He Nuclei and Electron Occurred</a>; <a href="https://doi.org/10.48550/arXiv.1212.0883">10.48550/arXiv.1212.0883</a></li>
<li>Webber, W. R. and Cummings, A. C., el al. (2012) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20200204-090030437">Large periodic time variations of termination shock particles between ~0.5-20 mev and 6-14 mev electrons measured by the crs experiment on Voyager 2 as it crossed into the heliosheath in 2007: An example of freshly accelerated cosmic rays?</a>; <a href="https://doi.org/10.48550/arXiv.1208.2982">10.48550/arXiv.1208.2982</a></li>
<li>Webber, W. R. and Cummings, A. C., el al. (2012) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20200204-101907790">20-125 MeV/nuc cosmic ray carbon nuclei intensities between 2004-2010 in solar cycle #23 as measured near the earth, at voyager 2 and also in the heliosheath at voyager 1 - modulation in a two zone heliospehre</a>; <a href="https://doi.org/10.48550/arXiv.1202.2081">10.48550/arXiv.1202.2081</a></li>
</ul>