Abstract Particle acceleration by slow magnetosonic waves (SMW) has been systematically disregarded. We examine the real possibility of this mode for acceleration of solar electrons on basis to a quantitative analysis. Evaluations of the times scales involved in the phenomenon allow us to determine the conditions in the solar atmosphere where resonant acceleration by the slow MHD mode may occur.
Solar particle acceleration by slow magnetosonic waves
Advances in Space Research ; 13 , 9 ; 187-190
1993-01-01
4 pages
Article (Journal)
Electronic Resource
English
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