Heating of the solar coronal plasma by fast electron streams

Details Heating of the solar coronal plasma by fast electron streams Heating of the solar coronal plasma by fast electron streams

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56.1286l&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, Nov.-Dec. 1979, p. 1286-1292. In Russian.

Other

Energetic Particles, High Energy Electrons, Plasma Heating, Solar Corona, Conductive Heat Transfer, Energy Transfer, Faculae, Isotherms, Plasma Turbulence, Plasma-Particle Interactions

Scientific paper

The paper considers coronal heating above plage regions caused by the dissipation of plasma turbulence generated by energetic electron streams. The efficiency of energy transfer from electron streams to the background plasma is estimated; it is shown that during developed storm bursts a layer of nonisothermal plasma is formed above the plage regions. Finally, the role of heat conductivity during the formation of such layers is discussed.

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