On the two-parameter models for stellar coronae

Details On the two-parameter models for stellar coronae On the two-parameter models for stellar coronae

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....78...36m&link_type=abstract

Astronomy and Astrophysics, vol. 78, no. 1, Sept. 1979, p. 36-38.

Astronomy and Astrophysics

Astrophysics

9

Atmospheric Heating, Shock Heating, Stellar Coronas, Stellar Models, Chromosphere, Conductive Heat Transfer, Energy Dissipation, Thermal Conductivity

Scientific paper

The two-parameter model developed by Hearn (1975) is reconsidered. A constraint required within the framework of such models is found which is not consistent, in general, with the minimum-flux condition conjectured by Hearn and which provides an alternative reduction of the models to one parameter. The corresponding relations are given explicitly for the special case of heating by weak shock waves when heat conduction back to the chromosphere dominates the energy losses by the corona.

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