Heavy ion composition in solar flares at low energies, 1973-1977

Details Heavy ion composition in solar flares at low energies, 1973-1977 Heavy ion composition in solar flares at low energies, 1973-1977

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icrc....5..110m&link_type=abstract

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

Computer Science

Abundance, Heavy Ions, Ion Temperature, Solar Cosmic Rays, Solar Flares, Explorer 50 Satellite, Particle Acceleration, Solar Flux

Scientific paper

The composition of solar flare particles near 1 MeV/nucleon has been surveyed for the major species between H and Fe over a four-year period using the IMP-8 ULET instrument. The average composition for the larger flares is found to be remarkably similar to that found by previous studies at energies greater than 10 MeV/nucleon. Variations in abundance are found to be well ordered by atomic number. It is suggested that such a smooth variation in abundances is due to an acceleration mechanism which preserves the main features of the ambient composition of the accelerated material, at least in the larger flares.

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