Abstract
By means of multi-dimensional radiative transfer calculations in inhomogeneous configurations representative of the solar chromosphere we investigate how the radiative energy losses in the K line of Ca II deviate from the plane-parallel case as the horizontal structural length of the assumed inhomogeneous scenario diminishes.
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© 1991 Springer Science+Business Media Dordrecht
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Fabiani, P., Bueno, J.T. (1991). On the Influence of Multi-Dimensional Radiative Transfer on the Energetic Contribution of the Ca K Line. In: Crivellari, L., Hubeny, I., Hummer, D.G. (eds) Stellar Atmospheres: Beyond Classical Models. NATO ASI Series, vol 341. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3554-2_40
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DOI: https://doi.org/10.1007/978-94-011-3554-2_40
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