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.
Cite
CITATION STYLE
APA
Pekünlü, R. (1999). Solar Flares. Turkish Journal of Physics, 23(2), 415–423. https://doi.org/10.1017/s0252921100034461
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