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Quasi–Static Evolution of Force–Free Magnetic Fields and a Model for Two–Ribbon Solar Flares
Published online by Cambridge University Press: 04 August 2017
Abstract
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We show that a sheared 2–D force–free field can evolve in a quasi–static way towards an open configuration, and apply this result to a qualitative theory of two–ribbon solar flares.
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- Session III
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- Copyright © Reidel 1985
References
Birn, J. and Schindler, K., 1981, Chap. 6 in
“Solar Flare Magnetohydrodynamics,”
Priest, E. R., Ed., Gordon and Breach, New York.Google Scholar
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