The observed characteristics of flare energy release. I - Magnetic structure at the energy release site
It is shown that flaring activity as seen in X-rays usually encompasses two or more interacting magnetic bipoles within an active region. Soft and hard X-ray spatiotemporal evolution is considered as well as the time dependence of the thermal energy content in different magnetic bipoles participatin...
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Veröffentlicht in: | Astrophys. J.; (United States) 1988-03, Vol.326 (1), p.425-450 |
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Sprache: | eng |
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