Abstract
The emission coefficient of the solar matter in the chromosphere has been calculated by Cox and Daltabuit (1971):
where f(T) is a numerically calculated function, ne and nH are the electron and the hydrogen densities.
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References
Cox, D.; Daltabuit, E.: 1971, Astrophys. J. 167, 113.
Kulsrud, R.: 1955, Astrophys. J. 121, 461.
Marik, M.: 1966, Astron. Zh. 43, 400.
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Osterbrock, D.: 1961, Astrophys. J. 134, 347.
Pikelner, S; Lifshitz, M.: 1964, Astron. Zh. 41, 1007.
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© 1982 D. Reidel Publishing Company
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Marik, M. (1982). A Theoretical Model of the Solar Chromosphere over a Suns Pot. In: Fricke, W., Teleki, G. (eds) Sun and Planetary System. Astrophysics and Space Science Library, vol 96. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7846-1_28
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DOI: https://doi.org/10.1007/978-94-009-7846-1_28
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