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Strong convective and shock wave behavior in solar flares
Authors:HW Bloomberg  J Davis  JP Boris
Institution:Science Applications, Inc., McLean, VA 22101, U.S.A.;Plasma Dynamics Branch, Naval Research Laboratory, Washington, DC 20375, U.S.A.
Abstract:A model has been developed to study the gasdynamics of a flare region heated by a stream of energetic electrons. It is shown that the energy deposition can introduce strong chromospheric dynamical effects. As a result of fluid motion into rarefield regions, there is considerable redistribution of mass causing a profound influence on the emitted line radiation.
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