Abstract Observational evidence that the plasma in hot X-ray sources in solar flares is highly turbulent is presented. The turbulent flare kernels are considered to be the main source of the flare energy release. Properties of kernels in big flares are discussed.
Investigation of turbulent kernels in solar flares
Advances in Space Research ; 11 , 5 ; 99-102
1991-01-01
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Converging motion of conjugate flaring kernels during two large solar flares
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