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..159q&link_type=abstract

Solar Physics, Volume 102, Issue 1-2, pp. 159-164

Physics

2

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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