Impulsive Flare Material: A Seed Population for Large Solar Particle Events?

Details Impulsive Flare Material: A Seed Population for Large Solar Particle Events? Impulsive Flare Material: A Seed Population for Large Solar Particle Events?

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3229m&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

8

Scientific paper

It has been suggested that gradual solar energetic particle (SEP) events enriched in 3 He and Fe result from the shock acceleration of remnant interplanetary material from previous impulsive flares. We test this hypothesis by comparing the number densities of Fe ions during quiet periods, 3 He-rich periods, and Ferich SEP events. We find that there is not a sufficient density of suprathermal Fe during typical quiet periods (or 3 He-rich periods) to account for the overall enrichment of Fe in and suggest other possibilities for interpreting these events.

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