Thermal equilibria of coronal magnetic loops with non-constant cross-sectional area

Details Thermal equilibria of coronal magnetic loops with non-constant cross-sectional area Thermal equilibria of coronal magnetic loops with non-constant cross-sectional area

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132..293s&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, April 1991, p. 293-306. SERC-supported research.

Physics

4

Coronal Loops, Solar Magnetic Field, Solar Temperature, Thermodynamic Equilibrium, Approximation, Solar Physics, Temperature Distribution

Scientific paper

Equations of thermal equilibrium along coronal loops are solved in the absence of gravity but where the cross-sectional area changes along the loop. The footpoint temperature is assumed to be 20,000 K. Several fundamental types of solution are found, namely hot loops, cool loops, hot-cool loops (where the footpoints and summits are cool but the intermediate parts are hotter) and warm loops (cool along most of their lengths except the summits).

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