Thermally isolated coronal loops in hydrostatic equilibrium

Details Thermally isolated coronal loops in hydrostatic equilibrium Thermally isolated coronal loops in hydrostatic equilibrium

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...80..309w&link_type=abstract

Solar Physics, vol. 80, Oct. 1982, p. 309-312. Research supported by the Science Research Council.

Physics

5

Coronal Loops, Hydrostatic Pressure, Plasma Equilibrium, Gravitational Effects, Temperature Effects

Scientific paper

Numerical solutions for the summit temperature and heating in a thermally isolated coronal loop in hydrostatic equilibrium are presented. The extent to which gravity modifies the normal uniform-pressure scaling law is shown, and plots of the differential emission measure are given. The base temperature chosen is 20,000 K. It is noted that while in principle the form of the heating affects the temperature profile, in practice (as a consequence of the present observation errors and the insensitivity of the energy balance models) it has not been possible to deduce much about the form of the coronal heating function.

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