Solar Flares

Authors : Rennan PEKÜNLÜ

Pages : 415-424

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Publication Date : 0000-00-00

Article Type : Research Paper

Abstract :In this paper, the dynamics, the magnetohydrodynamics and the energetics of flaring magnetic loops are reviwed. It is also emphasized that the presented model is in no way a unique one. The most commonly occurring type is labelled as B type flares. This paper reviews the general features of a B type flare.
Keywords : Turk J Phys, 23, 1999, , 415 424 Turk J Phys, vol 23, iss 2