Transition zone effects on thermal non-equilibrium and plasma condensation in solar coronal loops

Details Transition zone effects on thermal non-equilibrium and plasma condensation in solar coronal loops Transition zone effects on thermal non-equilibrium and plasma condensation in solar coronal loops

Aug 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...164..364s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 164, no. 2, Aug. 1986, p. 364-372.

Astronomy and Astrophysics

Astrophysics

10

Coronal Loops, Hydrodynamics, Nonequilibrium Thermodynamics, Plasma Layers, Chromosphere, Dense Plasmas, Lines Of Force, Magnetic Flux, Numerical Integration, Solar Magnetic Field

Scientific paper

The quasi-static thermal structure of arches or loops in the solar corona is investigated analytically, integrating the classical HD equations numerically along the magnetic-field lines and taking the effect of the transition region joining the arches to the chromosphere into account. Expressions for determining the mechanical heating rate and summit temperature from the footpoint chromospheric density and the loop length are obtained, and the implications of a solution with a cold dense mass sheet at the arcade summit are explored.

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