Energy equilibrium in coronal magnetic loops - reinvestigated

Details Energy equilibrium in coronal magnetic loops - reinvestigated Energy equilibrium in coronal magnetic loops - reinvestigated

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.222....9c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 222, no. 1-2, p. 9-38

Astronomy and Astrophysics

Astrophysics

Apexes, Coronal Holes, Lines Of Force, Magnetohydrostatics, Temperature Distribution, Temperature Gradients, Chromosphere, Conductive Heat Transfer, Electron Density (Concentration), Magnetic Fields

Scientific paper

Temperature distribution in cylindrically symmetric coronal magnetic loops has been reinvestigated under various conditions: (a) loop with the pressure varying along the radial distance, and (b) loop with constant pressure, for cooler apex loops and hotter apex loops. This work is reinvestigation of our previous work (Chandra and Prasad, 1993b).

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