A classification scheme for solar flare models |
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| Authors: | D S Spicer J C Brown |
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| Institution: | (1) Institute for Physical Science and Technology, University of Maryland, 20740 College Park, Md., U.S.A.;(2) E. O. Hulbert Center for Space Research, U.S. Naval Research Laboratory, 20375 Washington, D.C., U.S.A.;(3) Department of Astronomy, University of Glasgow, G12 8QQ Glasgow, Scotland, U.K. |
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| Abstract: | We present a classification scheme for solar flare models that utilize magnetic free energycurrents. The classification scheme is geometry independent and delineates models into two categories: those models utilizing currents flowing parallel to B and those utilizing currents flowing perpendicular to B. This delineation of drivers allows us to specify what kinds of plasma-magnetic field configurations should be expected for a given current driver. Further, the delineation of drivers will allow us to identify both the strengths and the weaknesses of the various models.Based on invited talks given at the SERF Workshop (Aug. 13, 1979) and the IAU Meeting of Commission 10 (Aug. 15, 1979) held in Montreal. |
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