Annotation
It is shown that the coronal source of hard X-ray radiation of a solar flare is produced in the collision of the plasma stream from a reconnecting current layer with a magnetic obstacle. The accumulation of reconnected magnetic flux behind the wave front explains the observed source motion velocity.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
S.A. Bogachev, B.V. Somov
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
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