The stabilizing effect of a transverse magnetic field in the current sheets of solar flares

Details The stabilizing effect of a transverse magnetic field in the current sheets of solar flares The stabilizing effect of a transverse magnetic field in the current sheets of solar flares

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..716v&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Aug. 1987, p. 716-722. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Current Sheets, Magnetic Field Configurations, Magnetohydrodynamic Stability, Plasma-Electromagnetic Interaction, Solar Flares, Solar Magnetic Field, Stellar Models, Tearing Modes (Plasmas)

Scientific paper

During the 'main' or 'hot' phase of solar flares, quasi-stationary
high-temperature current sheets are the energy source for the flares. It
is shown that these sheets are stabilized relative to tearing
instability by the small transverse magnetic-field component existing
within them.

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