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1999
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.
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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.
openaire +1 more source
Magnetic reconnection in solar flares
Geophysical and Astrophysical Fluid Dynamics, 1991T G Forbes
exaly
Contributions of the solar ultraviolet irradiance to the total solar irradiance during large flares
Journal of Geophysical Research, 2006Thomas Woods, Phillip Chamberlin
exaly
Ionospheric effects of solar flares at Mars
Geophysical Research Letters, 2009Sachchidanand Singh
exaly