Derivation of atmospheric structure from emission-line fluxes

Details Derivation of atmospheric structure from emission-line fluxes Derivation of atmospheric structure from emission-line fluxes

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.214p...1j&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 214, May 1, 1985, p. 1P-4P.

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Atmospheric Pressure, Atmospheric Temperature, Emission Spectra, Line Spectra, Stellar Atmospheres, T Tauri Stars, Chromosphere, Computational Astrophysics, Spectral Energy Distribution, Vertical Distribution

Scientific paper

In the present consideration of the way in which the pressure and temperature gradient in a stellar chromosphere and corona are related to the emission temperature distribution, the conditions under which a simple approximation for the temperature vs height suggested by Lago, Penston and Johnstone (1985) is appropriate are critically discussed. It is concluded that such approximations are not generally appropriate, and are an insufficient basis on which to construct atmospheric models.

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