Physical processes determining the structure of stellar chromospheres. I

Details Physical processes determining the structure of stellar chromospheres. I Physical processes determining the structure of stellar chromospheres. I

Jun 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982poast..30..123m&link_type=abstract

Postepy Astronomii, vol. 30, Apr.-June 1982, p. 123-144. In Polish.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Chromosphere, Late Stars, Radiative Heat Transfer, Stellar Atmospheres, Atmospheric Physics, Hydrogen, K Stars, Line Spectra, Spectral Line Width, Wave Attenuation

Scientific paper

The principal sources of radiative losses in the chromospheres of F, G, and K stars are indicated, with particular attention given to the hydrogen continuum and intense and faint lines formed by different elements. Mechanisms of the heating of stellar chromospheres are examined, with emphasis on heating via the dissipation of acoustic and magnetohydrodynamic waves.

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