The observable spatio-temporal characteristics of the energy release in flares and their association with the magnetic environment and tracers of field dynamics are reviewed. The observations indicate that impulsive phase manifestations, like particle acceleration, may be related to the formation of neutral sheets at the interface between interacting bipoles, but that the site for the bulk of the energy release is within closed loops rather than at the interaction site.
Observed form and action of the magnetic energy release in flares
Advances in Space Research ; 6 , 6, 19
1986-01-01
Sonstige
Keine Angabe
Englisch
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