Energy Dispersion in Solar Ion Events over 4 Orders of Magnitude: SOHO/COSTEP and Wind/STICS

Details Energy Dispersion in Solar Ion Events over 4 Orders of Magnitude: SOHO/COSTEP and Wind/STICS Energy Dispersion in Solar Ion Events over 4 Orders of Magnitude: SOHO/COSTEP and Wind/STICS

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3309p&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

3

Scientific paper

The ma jority of solar particle events in the COSTEP observational range of 4 75 MeV/n reveals nucleon energy disp ersion (NED), implying a flare-associated particle acceleration mechanism. Towards lower energies, the situation changes somewhat. Only in a minority of solar energetic particle (SEP) events can the effect of NED be followed into the lower keV range. We analyse the reasons for the distinctly different types of particle transport of >10 keV suprathermal up to 100 MeV energetic ions and conclude that the mean free path depends on rigidity.

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