Cooling of a coronal flare loop through radiation and conduction

Details Cooling of a coronal flare loop through radiation and conduction Cooling of a coronal flare loop through radiation and conduction

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..108..411s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 108, no. 2, 1987, p. 411-414.

Physics

36

Conductive Heat Transfer, Plasma Cooling, Radiative Heat Transfer, Solar Corona, Solar Flares, Cooling, Density Distribution, Temperature Effects

Scientific paper

A simple method is proposed for a computation of the cooling of coronal
flare loops by radiation and conduction, for various temperatures,
densities, and lengths of the loops. The relative importance of
conductive and radiative losses is briefly discussed.

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