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- W2011621900 abstract "The steady motion in sunspot magnetic regions is considered for both current-free and force-free configurations. The sufficient condition for stability is obtained in the presence of both external current-free and force-free magnetic fields and a steady motion. It is shown that the pattern of such steady motion is most important in triggering an instability of sunspot magnetic fields, both for the current-free and force-free configuration. When there is no steady motion, the current-free configuration of sunspot magnetic fields is always stable, whereas the stability in the case of force-free magnetic fields is connected with the configuration. The onset of a solar flare seems to be associated with an instability connected to the steady motion within the sunspot magnetic regions." @default.
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- W2011621900 date "1971-10-01" @default.
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- W2011621900 title "The stability of sunspot magnetic fields and the origin of solar flares" @default.
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- W2011621900 doi "https://doi.org/10.1016/0032-0633(71)90183-8" @default.
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