Numerical Simulation of a Solar Flare Produced by the Emergence of New Magnetic Flux

Details Numerical Simulation of a Solar Flare Produced by the Emergence of New Magnetic Flux Numerical Simulation of a Solar Flare Produced by the Emergence of New Magnetic Flux

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001arep...45...60p&link_type=abstract

Astronomy Reports, Volume 45, Issue 1, January 2001, pp.60-66

Astronomy and Astrophysics

Astronomy

8

Scientific paper

A scenario for the production of a current sheet above an active region during the emergence of new magnetic flux is considered. The formation of a current sheet is demonstrated via a numerical solution of a system of MHD equations with dissipative terms. The flare energy is stored in the magnetic field of the current sheet. The decay of the current sheet can account for a number of solar-flare phenomena, including the observed divergence of H α ribbons.

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