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
1990-01-01
5 pages
Article (Journal)
Electronic Resource
English
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