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Particle Acceleration by Magnetosonic Waves in a Coronal Loop
Published online by Cambridge University Press: 27 September 2017
Abstract
A model for the acceleration of electrons in a flaring coronal loop is described. The mechanism is stochastic acceleration by resonant interactions with a spectrum of conipressive magnetosonic waves. Current results of test particle calculations examining the feasibility of this model are presented.
- Type
- Session III: Theory
- Information
- International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 317 - 320
- Copyright
- Copyright © Kluwer 1989