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Quasi-Static Evolution of a Force-Free Magnetic Field Applications to the Theory of Stellar Flares and Coronal Heating.

机译:无磁场的准静态演化应用于恒星耀斑和冠状加热理论。

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摘要

We consider, in the highly conducting half-space, an x-invariant arcade force-free field which is evolving in a quasi-static way as a consequence of a velocity field imposed on a boundary plane. We show in particular that, when the shear exceeds a critical value, the configuration becomes metastable with respect to non-linear perturbations which change the topology of the field lines, but preserve the magnetic fluxes. (ERA citation 13:041642)

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