Observations of the temporal evolution of loop BC in soft X-rays in the November 5, 1980 flare are reviewed. Calculations are performed to model this evolution. The most consistent interpretation involving a minimum amount of energy is the following: thermal heating near B gives rise to a conduction front which moves out along the loop uninhibited for about 27 s, and beam heating near C gives rise to a second conduction front which moves in the opposite direction and prevents any energy reaching C by thermal conduction from B.
The relative contribution of beam versus thermally produced X-rays in the large loop of the 5 November 1980 flare
Advances in Space Research ; 6 , 6 19
1986-01-01
Sonstige
Keine Angabe
Englisch
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