Hydrodynamic shock wave formation in the solar chromosphere and corona during flares

Details Hydrodynamic shock wave formation in the solar chromosphere and corona during flares Hydrodynamic shock wave formation in the solar chromosphere and corona during flares

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ssrv...32...27s&link_type=abstract

(Slovenska Akademia Vied, IAU, and COSPAR, Study of Travelling Interplanetary Phenomena Workshop on Shock Waves in the Solar Cor

Physics

7

Hydrodynamics, Magnetic Field Reconnection, Magnetohydrodynamic Flow, Shock Waves, Solar Atmosphere, Solar Flares, Atmospheric Heating, Chromosphere, Shock Wave Propagation

Scientific paper

Consideration of the mechanisms of hydrodynamic shock wave formation in the solar atmosphere during flares establishes that hydrodynamic plasma flows during flares arise by means of fast energy release, after accumulation in solar atmosphere current magnetic fields, while shock waves arise through rapid heating of the chromospheric upper layers by accelerated particles or heat fluxes. Powerful hydrodynamic phenomena can also emerge, through the effect of an explosive current sheet disruption in the region of strong magnetic field reconnection. Shock wave formation and propagation in a nonhomogeneous and emitting solar atmosphere are discussed.

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