Model of a quasi-steady current sheet in the solar corona

Details Model of a quasi-steady current sheet in the solar corona Model of a quasi-steady current sheet in the solar corona

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..910p&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, Nov.-Dec. 1988, p. 910-916. In Russian.

Physics

Current Sheets, Plasma Dynamics, Solar Corona, Solar Flares, Solar Magnetic Field, Current Density, Electric Fields, Solar Wind

Scientific paper

The paper develops a model of a current sheet generated by a plasma flow in the vicinity of a single magnetic field line. A decrease in the total mass of the plasma in the sheet leads to the redistribution of plasma density; the density in the near zone decreases, which is necessary for the rapid restructuring of the magnetic field in the sheet. A solar-flare mechanism connected with this type of current sheet is considered.

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