First-order shock acceleration in solar flares

Details First-order shock acceleration in solar flares First-order shock acceleration in solar flares

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....4....6e&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 4 p 6-9 (SEE N85-34729 23-92)

Statistics

Astronomical Models, Fermi-Dirac Statistics, Particle Acceleration, Shock Wave Propagation, Solar Flares, Particle Diffusion, Particle Energy

Scientific paper

The first order Fermi shock acceleration model is compared with specific observations where electron, proton, and alpha particle spectra are available. In all events, it is found that a single shock with a compression ratio as inferred from the low energy proton spectra can reasonably produce the full proton, electron, and alpha particle spectra. The model predicts that the acceleration time to a given energy will be approximately equal for electrons and protons and, for reasonable solar parameters, can be less than 1 sec to 100 MeV.

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