Classic thermal conductivity in solar flares

Details Classic thermal conductivity in solar flares Classic thermal conductivity in solar flares

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18..296o&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 296; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 8, p. 731-734. In R

Astronomy and Astrophysics

Astronomy

Solar Flares, Thermal Conductivity, Heat Flux, Solar Atmosphere, Solar Temperature

Scientific paper

It is shown that classic thermal conductivity has a dominant effect on
solar flare processes. On the basis of an analysis of a large body of
observational data, the temperature conductivity coefficient is
estimated to be about 3 x 10 exp 15 sq cm/s.

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