Classical and anomalous heat conduction in solar flares

Details Classical and anomalous heat conduction in solar flares Classical and anomalous heat conduction in solar flares

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5...50s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Jan. 1979, p. 50-53.) Soviet Astronomy Letters, vol. 5, Jan.-Feb. 1979, p. 28-30. Tr

Astronomy and Astrophysics

Astronomy

Conductive Heat Transfer, Radiative Transfer, Solar Flares, Solar Wind, Approximation, Heat Flux, Plasma Heating, Pulse Heating, Temperature Dependence, Temperature Distribution

Scientific paper

Radiative cooling and heat conduction along the magnetic field will
determine the thermal structure of the plasma in solar flares. In either
gradual, continuous heating or rapid, pulsed heating, temperature
distributions will be established such that one may always employ the
classical approximation of collisional heat conduction.

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