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The importance of photospheric magnetic field complexity for coronal energy storage
Authors:W Van Tend
Institution:(1) The Astronomical Institute at Utrecht, Sterrewacht, Zonnenburg 2, 3512 Utrecht, NL, The Netherlands
Abstract:Possibilities for the storage of energy in coronal electric currents in different magnetic background field configurations are investigated in the framework of the solar flare energy build-up model of Van Tend and Kuperus (1978). The results are compared to characteristics of filaments and X-ray loops. Empirical flare predictors are interpreted theoretically.
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