Proton gyroresonance with parallel waves in a low-beta solar flare plasma

Details Proton gyroresonance with parallel waves in a low-beta solar flare plasma Proton gyroresonance with parallel waves in a low-beta solar flare plasma

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aipc..264..235s&link_type=abstract

In: Particle acceleration in cosmic plasmas; Proceedings of the Workshop, Bartol Research Inst., Newark, DE, Dec. 4-6, 1991 (A93

Computer Science

5

Plasma Resonance, Plasma Waves, Solar Flares, Solar Protons, Wave-Particle Interactions, Diffusion Coefficient, Fokker-Planck Equation

Scientific paper

We consider the gyroresonant interaction of protons with parallel electromagnetic plasma waves. These waves have either right- or left-hand circular polarization and include as a subset Alfven and whistler waves. We identify three comoving gyroresonances, which can lead to divergences in the Fokker-Planck coefficients. Taking into account thermal damping, we calculate the Fokker-Planck coefficient along with momentum diffusion coefficient D(p) and the mean-free path. Resulting acceleration time scales are compared with solar flare observations.

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