Investigations of X-raya spectra of solar flares show that intense random (turbulent) motions are present in hot flare plasma. Here it is argued that the turbulent motions are of great importance for flare development. They can efficiently enhance flare energy release and accelerate particles to high energies.
Investigations of turbulent motions and particle acceleration in solar flares
Advances in Space Research ; 6 , 6, 19
1986-01-01
Miscellaneous
No indication
English
Investigations of turbulent and directed motions in solar flares
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