The isotopic abundances of neon, magnesium and silicon nuclei accelerated in solar flares

Details The isotopic abundances of neon, magnesium and silicon nuclei accelerated in solar flares The isotopic abundances of neon, magnesium and silicon nuclei accelerated in solar flares

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5...85d&link_type=abstract

In: International Cosmic Ray Conference, 16th, Kyoto, Japan, August 6-18, 1979, Conference Papers. Volume 5. (A81-12386 02-93) T

Physics

Nuclear Physics

Abundance, Magnesium Isotopes, Neon Isotopes, Nuclei (Nuclear Physics), Silicon Isotopes, Solar Flares, Histograms, Solar Physics

Scientific paper

Direct measurements of the relative abundance of the isotopes Ne-20 and Ne-22 are reported along with a preliminary value for the Mg-26/Mg-24 ratio and an upper limit to the abundance of Si-30 in solar flare accelerated nuclei. A Ne-20/Ne-22 ratio of 7.7 plus 2.3 or minus 1.7 is in agreement with the ratio for the component Neon-A found in carbonaceous chondrites, while a preliminary value of 0.22 plus or minus 0.07 for Mg-26/Mg-24 is larger by approximately one standard deviation than the expected ratio of 0.14 given by Cameron (1973).

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