Journals / Turkish Journal of Physics / 1999 / Cilt: 23 - Sayı: 2

Solar Flares

Pages
415–423
DOI
—

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.

Özet

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. Full text: pdf Other articles published in the same issue: Turk. J. Phys., vol.23, iss.2.