Isotope abundances of solar coronal material derived from solar energetic particle measurements

Details Isotope abundances of solar coronal material derived from solar energetic particle measurements Isotope abundances of solar coronal material derived from solar energetic particle measurements

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...337..959m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 337, Feb. 15, 1989, p. 959-963.

Other

26

Abundance, Neon Isotopes, Particle Energy, Solar Corona, Carbon Isotopes, Fractionation, Magnesium Isotopes, Nitrogen Isotopes, Oxygen Isotopes

Scientific paper

Coronal isotopic abundances for the elements He, C, N, O, Ne, and Mg are derived from previously published measurements of the isotopic composition of solar energetic particles by first measuring, and then correcting for, the charge-to-mass-dependent fractionation due to solar flare acceleration and propagation processes. The resulting coronal composition generally agrees with that of other samples of solar system material, but the previously noted difference between the solar flare and solar wind Ne-22/Ne-20 ratios remains unresolved.

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