Physics
Scientific paper
Sep 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..339t&link_type=abstract
(Advanced School of Astronomy, Course on the Sun, a Tool for Stellar Physics, 6th, Erice, Italy, Aug. 8-21, 1976.) Società Astro
Physics
1
Stellar Atmospheres, Interstellar Matter, Nonequilibrium Thermodynamics, Solar Atmosphere, Solar Physics, Stellar Structure
Scientific paper
The nonequilibrium thermodynamic basis for modeling a stellar structure, subatmosphere, and atmosphere is formulated, along with the thermodynamic characterization of a star as a concentration of matter and energy in the interstellar medium. The analytical formulation of nonequilibrium thermodynamic models is discussed in the case where the nonisothermal storage modes are kinetic modes.
Thomas Nicholas R.
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