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Publisher
Springer, New York, NY
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Authors: Boris V Somov
Publish Date: 2013
Volume: , Issue: , Pages: 59-85
Abstract
Among a variety of kinetic phenomena related to fast particles in astrophysical plasma the simplest effect is Coulomb collisions under propagation of the particles in a plasma The socalled thicktarget model is considered An important role of the reversecurrent electric field in this model is demonstrated In particular we inevitably have to take into account the reverse current effects in order to study the problem of acceleration of electrons in solar flares However this problem is of general astrophysical significance how to interpret the observed cosmic hard Xrays quantitatively correct
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