Computer Science
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990kfnt....6...38k&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 6, Jan.-Feb. 1990, p. 38-42. In Russian.
Computer Science
4
High Temperature Plasmas, Radiant Cooling, Solar Corona, Spatial Distribution, Atmospheric Models, Optical Thickness, Thermal Instability
Scientific paper
Solutions are obtained for the hydrostatic equations of a plane-parallel completely ionized solar atmosphere with an extended heating source and classical electron heat conductivity. The effect of alternation between hot and cold dense regions divided by heat-conducting fronts is demonstrated with a solution in the form of a spatially-periodical structure. A relation is found between the spatial period and the gas pressure and power of the source. It is shown that a decrease in radiative cooling coupled with an increase in heating temperature leads to a decrease in maximum temperature. Also, it is suggested that the formation of cold dense condensations may be a result of the thermal instability of coronal plasma with a heating source.
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