Cooling of a Coronal Flare Loop Through Radiation and Conduction
Abstract
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.
- Publication:
-
Solar Physics
- Pub Date:
- September 1987
- DOI:
- 10.1007/BF00214172
- Bibcode:
- 1987SoPh..108..411S
- Keywords:
-
- Conductive Heat Transfer;
- Plasma Cooling;
- Radiative Heat Transfer;
- Solar Corona;
- Solar Flares;
- Cooling;
- Density Distribution;
- Temperature Effects;
- Solar Physics;
- Radiation;
- Flare;
- Radiative Loss;
- Flare Loop;
- Coronal Flare