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- W2079553555 abstract "view Abstract Citations (40) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The charge and isotopic composition of Z = 6-14 cosmic ray nuclei at their source Webber, W. R. Abstract Using data from a cosmic ray charge-isotope telescope flown on balloons, both the charge and isotopic composition are determined of Z = 6-14 cosmic ray nuclei. A low abundance for the elements N and Ne in the cosmic ray source relative to solar cosmic rays is observed. For the isotopes, a cosmic ray source ratio Ne-22/Ne-20 is found that is 3.52 plus or minus 0.67 times the solar ratio, this enhancement being due in part to an enhancement of Ne-22 and in part to an underabundance of Ne-20. Also observed are possible enhancements of the Mg-26/Mg-24 ratio, which is 1.40 plus or minus 0.24 times the solar t ratio, and the C-13/C-12 ratio, which is 2.90 plus or minus 0.93 times the solar ratio. For Ne, the underabundance of this element, coupled with the overabundnace of the isotope Ne-22, is seen as providing an important new clue to the nucleosynthesis processes producing these differences. Publication: The Astrophysical Journal Pub Date: January 1982 DOI: 10.1086/159565 Bibcode: 1982ApJ...252..386W Keywords: Chemical Composition; Cosmic Rays; Cosmochemistry; Isotopic Enrichment; Abundance; Balloon-Borne Instruments; Carbon 12; Neon Isotopes; Nitrogen Isotopes; Nuclear Fusion; Solar Cosmic Rays; Solar System; Telescopes; Space Radiation full text sources ADS |" @default.
- W2079553555 created "2016-06-24" @default.
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- W2079553555 date "1982-01-01" @default.
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- W2079553555 title "The charge and isotopic composition of Z = 6-14 cosmic ray nuclei at their source" @default.
- W2079553555 doi "https://doi.org/10.1086/159565" @default.
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