Magnetic reconnection in high-temperature plasma of solar flares. III - Stabilizing effect of the transverse magnetic field in a non-neutral current sheet

Details Magnetic reconnection in high-temperature plasma of solar flares. III - Stabilizing effect of the transverse magnetic field in a non-neutral current sheet Magnetic reconnection in high-temperature plasma of solar flares. III - Stabilizing effect of the transverse magnetic field in a non-neutral current sheet

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117...89s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 117, no. 1, 1988, p. 89-95.

Physics

9

High Temperature Plasmas, Magnetic Field Reconnection, Magnetohydrodynamic Stability, Solar Flares, Tearing Modes (Plasmas), Collisionless Plasmas, Current Sheets, Magnetic Field Configurations, Plasma Turbulence

Scientific paper

Quasi-steady high-temperature current sheets are an energy source during
the 'main' or 'hot' phase of solar flares. Such sheets are shown to be
stabilized with respect to the tearing instability by a small transverse
component of magnetic field existing in the sheets.

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