Abstract Flare energy release (plasma heating) is investigated using simple model considerations and soft-X-ray observations. It is shown that in order to heat and maintain the large amount of flare plasma at the high temperature, T>10 MK, it is necessary that the plasma be in a turbulent state and the energy release occur over a significant part of the plasma volume.
Discussion of the role of turbulence for the flare energy release
Advances in Space Research ; 10 , 9 ; 109-113
01.01.1990
5 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Laboratory experiments on solar flare energy release
Elsevier | 1990
|Flare Energy Release in the Diffusion Region
British Library Conference Proceedings | 1994
|Evolution of flare ribbons and energy release
Online Contents | 2003
|Evolution of Flare Ribbons and Energy Release
British Library Conference Proceedings | 2003
|Investigation of the Energy Release in Flare Kernels
British Library Conference Proceedings | 2002
|