Solar wind, non-force-free magnetic field and two-ribbon flares

Details Solar wind, non-force-free magnetic field and two-ribbon flares Solar wind, non-force-free magnetic field and two-ribbon flares

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..102..159s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 102, no. 1-2, Dec. 1985, p. 159-164.

Physics

2

Magnetic Field Configurations, Solar Flares, Solar Magnetic Field, Solar Physics, Solar Wind, Lines Of Force, Magnetohydrostatics, Tearing Modes (Plasmas)

Scientific paper

With the assumption that the magnetic field lines are radial at some quite high level in the solar corona, a non-constant shearing magnetic field is introduced into the magnetohydrostatic equations. It is found that a same critical amount of shearing a magnetic island is formed and then breaks out to form an open magnetic configuration in which resistive tearing-mode instability may occur, and may initiate a two-ribbon flare. In addition, high shearing magnetic fields are investigated. It is shown that high shearing magnetic configurations are weak two-dimensional neutral sheets, the instability of which has been studied by Janicke (1982).

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