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Electrostatically unstable heat flow during solar flares and its consequences
Authors:D. S. Spicer
Affiliation:(1) E. O. Hulburt Center for Space Research, U.S. Naval Research Laboratory, 2037S Washington, D.C., USA;(2) Institute for Fluid Dynamics and Applied Mathematics, University of Maryland, 20742 College Park, Md., USA
Abstract:We examine some of the consequences of an electrostatically unstable return current associated with heat conduction during a solar flare. We note that an electrostatically unstable return current will lead to strong hydrodynamic effects and more rapid magnetic field thermalization, if reconnection is the source of primary energy release during a solar flare.
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