Energetic Particle Mean Free Path in the Wave Heated Solar Wind

Details Energetic Particle Mean Free Path in the Wave Heated Solar Wind Energetic Particle Mean Free Path in the Wave Heated Solar Wind

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3539v&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

Scientific paper

We present simple analytical expressions for the power spectrum of cascading Alfv´n waves and the resulting solar energetic particle (SEP) mean free e path in the solar wind. The model can repro duce the short coronal mean free path required for efficient acceleration of SEPs in coronal shock waves as well as a longer interplanetary mean free path required for a rapid propagation of the accelerated particles to 1 AU.

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