๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Influence of magnetic field structure on the conduction cooling of flare loops

โœ Scribed by S. K. Antiochos; P. A. Sturrock

Publisher
Springer
Year
1976
Tongue
English
Weight
388 KB
Volume
49
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

A simple model facilitates calculation of the influence of magnetic field configuration on the conduction cooling rate of a hot post-flare coronal plasma. The magnetic field is taken to be that produced by a line dipole or point dipole at an arbitrary depth below the chromosphere. For the high temperatures (T~ > 10 7 K) produced by flares, the plasma may remain static and isobaric. The influence of the field is such as to increase the heat flux (per unit area) into the chromosphere, but to decrease the total conduction cooling of the flare plasma. This leads to a significant enhancement of the total energy radiated by the flare plasma.

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