Observational evidence and theoretical models for explosive mass motion in the impulsive phase of solar flares are reviewed. Data showing X-ray blueshifts and H-alpha redshifts are presented in graphs and diagrams and interpreted in terms of upward-moving material at 10 million K and downward-moving material at 10,000 K. This motion is found to be most simply explained in terms of explosive chromospheric evaporation.
Impulsive phase explosive dynamics
Advances in Space Research ; 6 , 6 19
1986-01-01
Sonstige
Keine Angabe
Englisch
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