Further isotopic studies of heavy nuclei in the 9/23/78 solar flare

Details Further isotopic studies of heavy nuclei in the 9/23/78 solar flare Further isotopic studies of heavy nuclei in the 9/23/78 solar flare

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4...42m&link_type=abstract

International Cosmic Ray Conference, 18th, Bangalore, India, Aug. 22-Sept. 3, 1983, Paper. 4 p.

Computer Science

Abundance, Heavy Nuclei, Solar Corpuscular Radiation, Solar Flares, Solar Wind, Isotopic Enrichment, Neon Isotopes

Scientific paper

The isotopes considered range from He to Mg (Z from 2 to 12). A more accurate value of the Ne-22/Ne-20 ratio is obtained by extending the energy interval for isotope analysis. A significant difference persists between the Ne-22/Ne-20 ratio in this flare and that for the solar wind. How the sun can apparently emit two distinct isotopic components remains a question. Although relatively little is known about the solar wind isotopic composition, it does not appear that the solar wind isotopes have been altered by a simple mass-dependent fractionation process. Reference is made to models that have been proposed which might produce selective enhancements.

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