The action of a compressing and shearing non-force-free magnetic field on the build-up and triggering of a two-ribbon flare

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The corresponding field configurations of the solar isothermal atmosphere obtained from a series of non-constant shearing magnetic fields after considering both the gravity and gas pressure are examined and compared. When the shearing magnetic field increases, magnetic islands will appear, followed by shearing, quasi-three-dimensional field structures approaching the open state, and with almost anti-parallel field lines. It is possible that this is related to the initial phase of a two-ribbon flare.

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