Possible MHD phenomena in flare processes on the sun

Details Possible MHD phenomena in flare processes on the sun Possible MHD phenomena in flare processes on the sun

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983maggi.......21v&link_type=abstract

Magnitnaia Gidrodinamika (ISSN 0025-0015), Apr.-June 1983, p. 21-24. In Russian.

Physics

Energy Transfer, Magnetohydrodynamic Flow, Solar Flares, Flow Velocity, Lines Of Force, Magnetic Field Configurations, Plasma Turbulence

Scientific paper

It is shown that the presence of inhomogeneous velocity structures in
plasma motions on the sun can lead to local intensification of magnetic
fields with subsequent reconnection. The rapid release of magnetic
energy occurs during the reconnection, the released energy ranging from
10 to the 19th J (small flares) to 10 to the 25th J (large flares).

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