Composition of energetic particles from solar flares

Details Composition of energetic particles from solar flares Composition of energetic particles from solar flares

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994adspr..14..589g&link_type=abstract

Advances in Space Research, vol. 14, no. 10, p. 589-598

Computer Science

16

Heavy Nuclei, Plasma Composition, Solar Flares, Solar Radiation, Corpuscular Radiation, Galileo Spacecraft, Linear Energy Transfer (Let), Radiation Measurement, Single Event Upsets

Scientific paper

We present a model for composition of heavy ions in the Solar Energetic Particles (SEP). The SEP composition in a typical large solar particle event reflects the composition of the Sun, with adjustments due to fractionation effects which depend on the First Ionization Potential (FIP) of the ion and on the ratio of ionic charge to mass (Q/M). Flare-to flare variations in composition are represented by parameters describing these fractionation effects and the distributions of these parameters are presented.

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