Impulsive Acceleration and Bulk Heating of Flare Plasma by Plasma Turbulence

Physics

Scientific paper

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Scientific paper

A new paradigm of the non-thermal thick target model for the impulsive phase of solar flares is described, where plasma waves or turbulence play a major role in the acceleration of particles and a prominent role in the impulsive heating of footpoints of flare loops, as is seen in the January 26, 1992 flare by YOHKOH. This modification makes the required energy and physical conditions more reasonable and has an important bearing on the heating of the corona and the Neupert effect.

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