Energy balance in the prominence-corona transition region

Details Energy balance in the prominence-corona transition region Energy balance in the prominence-corona transition region

Mar 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991soph..132...81c&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 132, March 1991, p. 81-94.

Physics

27

Energy Budgets, High Temperature Plasmas, Solar Corona, Solar Magnetic Field, Solar Prominences, Solar Radio Emission, Temperature Gradients, Ultraviolet Radiation

Scientific paper

The prominence-corona transition region can be observed both at UV and radio wavelengths. The physical parameters needed to explain one set of observations are, however, in disagreement with those consistent with the other one. A solution of the problem is proposed, based on the proper consideration of the dependence of the thermal conduction on the angle between the magnetic field and the direction of the local temperature gradient.

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