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.
PEKÜNLÜ, E. RENNAN (1999) "Solar Flares," Turkish Journal of Physics: Vol. 23: No. 2, Article 13. Available at: https://journals.tubitak.gov.tr/physics/vol23/iss2/13