Strong convective and shock wave behavior in solar flares

Details Strong convective and shock wave behavior in solar flares Strong convective and shock wave behavior in solar flares

Aug 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977jqsrt..18..237b&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer, vol. 18, Aug. 1977, p. 237-244. Navy-supported research;

Physics

3

Shock Heating, Solar Flares, Solar Temperature, Stellar Models, Chromosphere, Electron Energy, Particle Acceleration, Solar Electrons

Scientific paper

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 rarefied regions, there is considerable redistribution of mass causing a profound influence on the emitted line radiation.

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