Title: Radiative transfer in two-component stellar atmospheres
Abstract: We describe a method for solving the line-transfer equations for a two-component atmosphere consisting of an array of columns, characterized by a particular variation of temperature with height, which are embedded in a medium in which the temperature is a different function of height. Radiative interaction between the two regions is taken into account, and the opacity is allowed to vary arbitrarily with depth. Some calculations that correspond to the solar Ca K-line are described.
Publication Year: 1971
Publication Date: 1971-06-01
Language: en
Type: article
Indexed In: ['crossref']
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Cited By Count: 9
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