On the energy balance of stellar coronae

Details On the energy balance of stellar coronae On the energy balance of stellar coronae

Mar 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....73..190e&link_type=abstract

Astronomy and Astrophysics, vol. 73, no. 1-2, Mar. 1979, p. 190-192.

Astronomy and Astrophysics

Astrophysics

20

Atmospheric Heating, Energy Budgets, Stellar Coronas, Stellar Models, Atmospheric Models, Atmospheric Temperature, Energy Dissipation, Graphs (Charts)

Scientific paper

From a survey of proposed coronal heating mechanisms, it is concluded that these processes not only provide a certain heating flux but also, through a damping length L, determine the mode of dissipation of this flux. Both for simplified and more elaborate models it is found that L determines both the magnitude and the position of the coronal temperature maximum. Such detailed determination of the corona model by the heating mechanism appears to contradict the concept of a minimum-flux corona.

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