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Do We Really Know What the Actual Chromospheric Heating Requirements Are?

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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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References

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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

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-642-87457-4

  • Online ISBN: 978-3-642-87455-0

  • eBook Packages: Springer Book Archive

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