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A model of impulsive loop flares revisited
Authors:D. F. Smith  S. H. Brecht
Affiliation:(1) Berkeley Research Associates, 290 Green Rock Drive, 80303 Boulder, CO, USA;(2) Department of Astrophysical, Planetary, and Atmospheric Sciences, University of Colorado, USA;(3) Berkeley Research Associates, P.O. Box 241, 94701 Berkeley, CA, USA
Abstract:A critical examination of the components of the recent impulsive loop flare model of Takakura is made. It is found that his analysis of the stability of the electron distribution resulting from anomalous heat conduction is in error and electron plasma waves would not be excited. Rather, in the regions where the electron/proton temperature ratioTe/Ti lap 10, electrostatic ion-cyclotron waves would be excited and in the regions whereTe gap 10, ion-acoustic waves would be excited. Ratios ofTe/Ti gap 10 occur only in the late time development behind the conduction fronts. Since the anomalous resistivity due to electrostatic ion-cyclotron waves is fortuitously about 70% of the one used by Takakura, the general development will follow closely the one calculated by him. Because the anomalous resistivity due to ion-acoustic waves is about 95 times the one used by Takakura, the development in the parts of the loop whereTe/Ti gap 10 for late times would be altered considerably.Also Guest Worker at NOAA Space Environment Laboratory, Boulder, Colorado, U.S.A.
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