Proc. IAU volume 13, issue S335, P90-93 2017 DOI: 10.1017/s1743921317008912 View full text
P. A. Gritsyk, B. V. Somov

Abstract: AbstractUsing the appropriate kinetic equation, we considered the problem of propagation of accelerated electrons into the solar corona and chromosphere. Its analytical solution was used for modelling the M7.7 class limb flare occurred on July 19, 2012. Coronal above-the-loop-top hard X-Ray source was interpreted in the thin-target approximation, the foot-point source - in the thick-target approximation with account of the reverse-current electric field. For the foot-point source we found a good accordance wit…

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