Abstract
By means of multi-dimensional radiative transfer calculations we show that the plane-parallel approximation begins to fail to give proper account of the energetic role of spectral lines when the stellar atmospheric inhomogeneities have horizontal structural lengths smaller than 1000 km.
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Anderson, L. S., Athay, R. G.: 1989, Astrophys. J. 336, 1089
Avrett, E. H.: 1985, in Chrom o spheric Diagnostics and Modelling, B. W. Lites (ed.), National Solar Observatory, Sunspot, N. M. 88349, p. 67
Stein, R. F.: 1985, in Chromospheric Diagnostics and Modelling, B. W. Lites (ed.), National Solar Observatory, Sunspot, N. M. 88349, p. 213
Trujillo Bueno, J., Kneer, F.: 1990, Astron. Astrophys. 232, 135
Vernazza, J. E., Avrett, E. H., Loeser, R.: 1981, Astrophys. J. Suppl. 45, 635
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© 1991 Springer-Verlag Berlin Heidelberg
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Bueno, J.T. (1991). Do We Really Know What the Actual Chromospheric Heating Requirements Are?. In: Ulmschneider, P., Priest, E.R., Rosner, R. (eds) Mechanisms of Chromospheric and Coronal Heating. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-87455-0_14
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DOI: https://doi.org/10.1007/978-3-642-87455-0_14
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