<h1>Israel, Martin Henry</h1>
<h2>Article from <a href="https://authors.library.caltech.edu">CaltechAUTHORS</a></h2>
<ul>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2022) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20220908-184327219">The Isotopic Abundances of Galactic Cosmic Rays with Atomic Number 29 ≤ Z ≤ 38</a>; Astrophysical Journal; Vol. 936; No. 1; 13; <a href="https://doi.org/10.3847/1538-4357/ac82e7">10.3847/1538-4357/ac82e7</a></li>
<li>Israel, M. H. and Lave, K. A., el al. (2018) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20180921-095050945">Elemental Composition at the Cosmic-Ray Source Derived from the ACE-CRIS Instrument. I. _6C to _(28)Ni</a>; Astrophysical Journal; Vol. 865; No. 1; Art. No. 69; <a href="https://doi.org/10.3847/1538-4357/aad867">10.3847/1538-4357/aad867</a></li>
<li>Murphy, R. P. and Sasaki, M., el al. (2016) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20161104-083553694">Galactic Cosmic Ray Origins and OB Associations: Evidence from SuperTIGER Observations of Elements _(26)Fe through _(40)Zr</a>; Astrophysical Journal; Vol. 831; No. 2; Art. No. 148; <a href="https://doi.org/10.3847/0004-637X/831/2/148">10.3847/0004-637X/831/2/148</a></li>
<li>Binns, W. R. and Israel, M. H., el al. (2016) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20160422-072602817">Observation of the ^(60)Fe nucleosynthesis-clock isotope in galactic cosmic rays</a>; Science; Vol. 352; No. 6286; 677-680; <a href="https://doi.org/10.1126/science.aad6004">10.1126/science.aad6004</a></li>
<li>Lave, K. A. and Wiedenbeck, M. E., el al. (2013) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20130725-072008737">Galactic Cosmic-Ray Energy Spectra and Composition during the 2009-2010 Solar Minimum Period</a>; Astrophysical Journal; Vol. 770; No. 2; Art. No. 117; <a href="https://doi.org/10.1088/0004-637X/770/2/117">10.1088/0004-637X/770/2/117</a></li>
<li>Mewaldt, R. A. and Davis, A. J., el al. (2010) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20101209-103120218">Record-setting Cosmic-ray Intensities in 2009 and 2010</a>; Astrophysical Journal Letters; Vol. 723; No. 1; L1-L6; <a href="https://doi.org/10.1088/2041-8205/723/1/L1">10.1088/2041-8205/723/1/L1</a></li>
<li>George, J. S. and Lave, K. A., el al. (2009) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20091009-094741170">Elemental Composition and Energy Spectra of Galactic Cosmic Rays During Solar Cycle 23</a>; Astrophysical Journal; Vol. 689; No. 2; 1666-1681; <a href="https://doi.org/10.1088/0004-637X/698/2/1666">10.1088/0004-637X/698/2/1666</a></li>
<li>Rauch, B. F. and Link, J. T., el al. (2009) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20090826-142040089">Cosmic Ray origin in OB Associations and Preferential Acceleration of Refractory Elements: Evidence from Abundances of Elements _(26)Fe through _(34)Se</a>; Astrophysical Journal; Vol. 697; No. 2; 2083-2088; <a href="https://doi.org/10.1088/0004-637X/697/2/2083">10.1088/0004-637X/697/2/2083</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2008) <a href="https://resolver.caltech.edu/CaltechAUTHORS:BINnar08">The OB association origin of galactic cosmic rays</a>; New Astronomy Reviews; Vol. 52; No. 7-10; 427-430; <a href="https://doi.org/10.1016/j.newar.2008.05.008">10.1016/j.newar.2008.05.008</a></li>
<li>Wiedenbeck, M. E. and Binns, W. R., el al. (2007) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20100909-133903373">An Overview of the Origin of Galactic Cosmic Rays as Inferred from Observations of Heavy Ion Composition and Spectra</a>; Space Science Reviews; Vol. 130; No. 1-4; 415-429; <a href="https://doi.org/10.1007/s11214-007-9198-y">10.1007/s11214-007-9198-y</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2007) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140827-105038224">OB Associations, Wolf-Rayet Stars, and the Origin of Galactic Cosmic Rays</a>; Space Science Reviews; Vol. 130; No. 1-4; 439-449; <a href="https://doi.org/10.1007/s11214-007-9195-1">10.1007/s11214-007-9195-1</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2006) <a href="https://resolver.caltech.edu/CaltechAUTHORS:BINjpcs06">Superbubbles, Wolf-Rayet stars, and the origin of galactic cosmic rays</a>; Journal of Physics: Conference Series; Vol. 47; 68-77; <a href="https://doi.org/10.1088/1742-6596/47/1/008">10.1088/1742-6596/47/1/008</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2006) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20110120-162201593">Wolf-Rayet stars, OB associations, and the origin
of galactic cosmic rays</a>; New Astronomy Reviews; Vol. 50; No. 7-8; 516-520; <a href="https://doi.org/10.1016/j.newar.2006.06.058">10.1016/j.newar.2006.06.058</a></li>
<li>Geier, S. and Barbier, L. M., el al. (2006) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20110601-134548173">A search for the signature of microquasars in the cosmic ray iron spectrum measured by TIGER</a>; Advances in Space Research; Vol. 37; No. 10; 1955-1959; <a href="https://doi.org/10.1016/j.asr.2005.10.037">10.1016/j.asr.2005.10.037</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2005) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140827-093644016">Cosmic-Ray Neon, Wolf-Rayet Stars, and the Superbubble Origin of Galactic Cosmic Rays</a>; Astrophysical Journal; Vol. 634; No. 1; 351-364; <a href="https://doi.org/10.1086/496959">10.1086/496959</a></li>
<li>Israel, M. H. and Binns, W. R., el al. (2005) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140826-114144077">Isotopic Composition of Cosmic Rays: Results from the Cosmic Ray Isotope Spectrometer on the ACE Spacecraft</a>; Nuclear Physics A; Vol. 758; 201-208; <a href="https://doi.org/10.1016/j.nuclphysa.2005.05.038">10.1016/j.nuclphysa.2005.05.038</a></li>
<li>Niebur, S. M. and Scott, L. M., el al. (2003) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140826-164919486">Cosmic ray energy loss in the heliosphere: Direct evidence from electron-capture-decay secondary isotopes</a>; Journal of Geophysical Research A; Vol. 108; No. A10; Art. No. 8033; <a href="https://doi.org/10.1029/2003JA009876">10.1029/2003JA009876</a></li>
<li>Yanasak, N. E. and Wiedenbeck, M. E., el al. (2001) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140827-082013151">Measurement of the Secondary Radionuclides ^(10)Be, ^(26)Al, ^(36)Cl, ^(54)Mn, and ^(14)C and Implications for the Galactic Cosmic-Ray Age</a>; Astrophysical Journal; Vol. 563; No. 2; 768-792; <a href="https://doi.org/10.1086/323842">10.1086/323842</a></li>
<li>Wiedenbeck, M. E. and Yanasak, N. E., el al. (2001) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140827-090214937">The Origin of Primary Cosmic Rays: Constraints from ACE Elemental and Isotopic Composition Observations</a>; Space Science Reviews; Vol. 99; No. 1-4; 15-26; <a href="https://doi.org/10.1023/A:1013816209004">10.1023/A:1013816209004</a></li>
<li>Binns, W. R. and Wiedenbeck, M. E., el al. (2001) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140826-133307053">Galactic cosmic ray neon isotopic abundances measured by the cosmic ray isotope spectrometer (CRIS) on ACE</a>; Advances in Space Research; Vol. 27; No. 4; 767-772; <a href="https://doi.org/10.1016/S0273-1177(01)00119-3">10.1016/S0273-1177(01)00119-3</a></li>
<li>Wiedenbeck, M. E. and Binns, W. R., el al. (2001) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140826-112434005">The isotopic source composition of cosmic-ray iron, cobalt, and nickel</a>; Advances in Space Research; Vol. 27; No. 4; 773-778; <a href="https://doi.org/10.1016/S0273-1177(01)00120-X">10.1016/S0273-1177(01)00120-X</a></li>
<li>Yanasak, N. E. and Wiedenbeck, M. E., el al. (2001) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140826-115932195">Cosmic-ray time scales using radioactive clocks</a>; Advances in Space Research; Vol. 27; No. 4; 727-736; <a href="https://doi.org/10.1016/S0273-1177(01)00114-4">10.1016/S0273-1177(01)00114-4</a></li>
<li>Cummings, J. R. and Binns, W. R., el al. (1990) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140501-111116037">Determination of the Cross Sections for the Production of Fragments from Relativistic Nucleus-Nucleus Interactions. Part II: Parametric Fits</a>; Physical Review C; Vol. 42; No. 6; 2530-2545; <a href="https://doi.org/10.1103/PhysRevC.42.2530">10.1103/PhysRevC.42.2530</a></li>
<li>Cummings, J. R. and Binns, W. R., el al. (1990) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140501-110735443">Determination of the Cross Sections for the Production of Fragments from Relativistic Nucleus-Nucleus Interactions. Part I: Measurements</a>; Physical Review C; Vol. 42; No. 6; 2508-2530; <a href="https://doi.org/10.1103/PhysRevC.42.2508">10.1103/PhysRevC.42.2508</a></li>
<li>Binns, W. R. and Garrard, T. L., el al. (1989) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140909-090921312">Abundances of ultraheavy elements in the cosmic radiation: results from HEAO 3</a>; Astrophysical Journal; Vol. 346; No. 2; 997-1009; <a href="https://doi.org/10.1086/168082">10.1086/168082</a></li>
<li>Binns, W. R. and Cummings, J. R., el al. (1989) <a href="https://resolver.caltech.edu/CaltechAUTHORS:BINprc89">Charge, mass, and energy changes during fragmentation of relativistic nuclei</a>; Physical Review C; Vol. 39; No. 5; 1785-1798; <a href="https://doi.org/10.1103/PhysRevC.39.1785">10.1103/PhysRevC.39.1785</a></li>
<li>Binns, W. R. and Garrard, T. L., el al. (1988) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140430-161225559">Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from _(18)Ar to _(28)Ni - Results from HEAO 3</a>; Astrophysical Journal; Vol. 324; No. 2; 1106-1117; <a href="https://doi.org/10.1086/165966">10.1086/165966</a></li>
<li>Binns, W. R. and Garrard, T. L., el al. (1987) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140219-131337968">Systematics of the release of residual nuclei from relativistic nucleus-nucleus interactions</a>; Physical Review C; Vol. 36; No. 5; 1870-1885; <a href="https://doi.org/10.1103/PhysRevC.36.1870">10.1103/PhysRevC.36.1870</a></li>
<li>Green, M. A. and Smoot, G. F., el al. (1987) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140430-091525676">ASTROMAG: A Superconducting Particle Astrophysics Magnet Facility for the Space Station</a>; IEEE Transactions on Magnetics; Vol. 23; No. 2; 1240-1243; <a href="https://doi.org/10.1109/TMAG.1987.1064905">10.1109/TMAG.1987.1064905</a></li>
<li>Binns, W. R. and Brewster, N. R., el al. (1985) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140408-134101988">Lead, platinum, and other heavy elements in the primary cosmic radiation - HEAO 3 results</a>; Astrophysical Journal; Vol. 297; No. 1; 111-118; <a href="https://doi.org/10.1086/163508">10.1086/163508</a></li>
<li>Binns, W. R. and Fixsen, D. J., el al. (1984) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140429-095757981">Elemental Abundances of Ultraheavy Cosmic Rays</a>; Advances in Space Research; Vol. 4; No. 2-3; 25-34; <a href="https://doi.org/10.1016/0273-1177(84)90289-8">10.1016/0273-1177(84)90289-8</a></li>
<li>Binns, W. R. and Fickle, R. K., el al. (1983) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140409-080134015">Cosmic-ray abundances of Sn, Te, Xe, and BA nuclei measured on HEAO 3</a>; Astrophysical Journal Letters; Vol. 267; No. 2; L93-L96; <a href="https://doi.org/10.1086/184010">10.1086/184010</a></li>
<li>Binns, W. R. and Fickle, R. K., el al. (1983) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140421-140007292">Cosmic Ray Abundances of Sn, Te, Xe, and Ba Nuclei Measured on HEAO 3</a>; Astrophysical Journal; Vol. 267; L93-L96</li>
<li>Binns, W. R. and Fickle, R. K., el al. (1982) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140304-105424511">The abundance of the actinides in the cosmic radiation as measured on HEAO 3</a>; Astrophysical Journal; Vol. 261; No. 2; L117-L120; <a href="https://doi.org/10.1086/183899">10.1086/183899</a></li>
<li>Binns, W. R. and Fickle, R. K., el al. (1981) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140417-151939075">Cosmic-Ray Abundances of Elements with Atomic Number 26 ≤ Z ≤ 40 Measured on HEAO-3</a>; Astrophysical Journal Letters; Vol. 247; No. 3; L115-L118; <a href="https://doi.org/10.1086/183602">10.1086/183602</a></li>
<li>Binns, W. R. and Fickle, R. K., el al. (1981) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140212-075813791">Cosmic-ray abundances of elements with atomic number 26 ≤ Z ≤ 40 measured on HEAO 3</a>; Astrophysical Journal; Vol. 247; No. 3; L115-L118; <a href="https://doi.org/10.1086/183602">10.1086/183602</a></li>
<li>Binns, W. R. and Israel, M. H., el al. (1981) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140417-142518040">The UH-Nuclei Cosmic Ray Detector on the Third High Energy Astronomy Observatory</a>; Nuclear Instruments and Methods; Vol. 185; No. 1-3; 415-426; <a href="https://doi.org/10.1016/0029-554X(81)91239-8">10.1016/0029-554X(81)91239-8</a></li>
<li>Israel, Martin H. (1969) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140407-083507912">Cosmic-Ray Electrons between 12 Mev and 1 Gev in 1967</a>; Journal of Geophysical Research A; Vol. 74; No. 19; 4701-4713; <a href="https://doi.org/10.1029/JA074i019p04701">10.1029/JA074i019p04701</a></li>
<li>Israel, Martin H. and Vogt, Rochus E. (1969) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140403-102131366">Characteristics of the Diurnally Varying Electron Flux Near the Polar Cap</a>; Journal of Geophysical Research A; Vol. 74; No. 19; 4714-4720; <a href="https://doi.org/10.1029/JA074i019p04714">10.1029/JA074i019p04714</a></li>
<li>Israel, Martin H. and Vogt, Rochus E. (1968) <a href="https://resolver.caltech.edu/CaltechAUTHORS:20140403-101033514">Flux of Cosmic Ray Electrons Between 17 and 63 MeV</a>; Physical Review Letters; Vol. 20; No. 19; 1053-1056; <a href="https://doi.org/10.1103/PhysRevLett.20.1053">10.1103/PhysRevLett.20.1053</a></li>
</ul>