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Particle Acceleration in Solar Flares

Published online by Cambridge University Press:  25 May 2016

J. A. Miller
J. A. Miller*
Affiliation:
Department of Physics, The University of Alabama in Huntsville, Huntsville, AL 35899, U.S.A.

Abstract

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We review the basic, observationally driven requirements for a successful model of particle acceleration in impulsive solar flares and then evaluate the viability of three classes of acceleration mechanisms. We argue that stochastic resonant acceleration is by far the most promising of the mechanisms.

Type
Part I: Talks
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 277 - 290
Copyright
Copyright © Astronomical Society of the Pacific 2000 

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