Elemental composition of solar energetic nuclei

Details Elemental composition of solar energetic nuclei Elemental composition of solar energetic nuclei

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238l..97c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 238, June 1, 1980, L97-L101.

Astronomy and Astrophysics

Astronomy

18

Abundance, Cosmic Rays, Energetic Particles, Photosphere, Solar Flares, Solar Wind, Solar Atmosphere, Solar Corona, Solar Flux, Spaceborne Astronomy, Voyager Project

Scientific paper

It is found for four major solar-flare events that the average solar energetic particle (SEP) abundances are similar to abundances in the solar wind and to recent coronal measurements. The average SEP and galactic cosmic-ray source abundances are also similar for elements with nuclear charge in the range 8-28, but are different for helium, carbon, and nitrogen.

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