A solar flare model including the formation and destruction of the current sheet in the corona

Details A solar flare model including the formation and destruction of the current sheet in the corona A solar flare model including the formation and destruction of the current sheet in the corona

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992soph..139..125p&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 139, no. 1, May 1992, p. 125-145.

Physics

25

Current Sheets, Solar Corona, Solar Flares, Stellar Models, Field Aligned Currents, Magnetic Storms, Magnetohydrodynamic Stability, Solar Magnetic Field, Solar Storms

Scientific paper

A numerical simulation method is used to show the possibility of forming a current sheet in the solar corona in an active region with four magnetic poles. The evolution of the quasi-stationary current sheet can lead to its transfer to an unsteady state. The MHD instability of this sheet causes its decay, accompanied by a set of events which characterizes the solar flare. The electrodynamical model of a solar flare includes a system of field-aligned currents typical of a magnetospheric substorm. Several events in substorms and solar flares are explained by the generation of field-aligned currents.

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