Ne-22 and the nature of low energy cosmic ray sources

Details Ne-22 and the nature of low energy cosmic ray sources Ne-22 and the nature of low energy cosmic ray sources

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.200..123r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 200, July 1982, p. 123-126. Research supported by the University of Pen

Other

Abundance, Cosmic Rays, Isotopic Enrichment, Neon Isotopes, Particle Energy, Radiation Sources, B Stars, Carbon 13, Novae, Nuclear Fusion, O Stars, Sodium 22, Solar Cosmic Rays

Scientific paper

The recent measurements on the isotopic abundances in cosmic rays of energy less than 500 MeV/n have confirmed the over-abundance of Ne-22 by more than a factor of three compared with the solar abundance. No comparable enhancements have been seen in the case of any other isotopes, especially that of C-13. This is shown to be in disagreement with the models in which cosmic rays originate in the grains from novae.

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