Publication Date:
2019-06-27
Description:
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.
Keywords:
SOLAR PHYSICS
Type:
Journal of Quantitative Spectroscopy and Radiative Transfer; 18; Aug. 197
Format:
text