Energy Spectra of Very Large Gradual Solar Particle Events

Details Energy Spectra of Very Large Gradual Solar Particle Events Energy Spectra of Very Large Gradual Solar Particle Events

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....8.3189t&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

Energy spectra provide a powerful tool in understanding solar energetic particle (SEP) events, in that spectra contain information on all aspects of SEP production, including source plasma, interplanetary transport effects, and characteristics of the accelerator. We compare energy spectra of two very large gradual events (1998 April 20 and 2000 July 14), produced by shocks driven by fast coronal mass ejections (CMEs). We show that differences in their Fe spectra can be understood in terms of a small, variable admixture of remant flare suprathermals in the SEP source population.

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