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Discussion on the Quiet Chromosphere

  • R. O. Redman
  • L. De Feiter
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 2)

Abstract

M. J. Seaton. I would like to ask Jefferies two questions:
  1. (1)

    The chromosphere theory has been expressed in terms of mathematical problems which are difficult but which are nonetheless soluble. But just how much error comes from the assumption of parallel stratified layers?

     
  2. (2)

    It has been explained that information on the source function can be obtained from studies of the components of a doublet. Would it not be possible to get good consistency checks using a triplet

     

Keywords

Optical Depth Brightness Temperature Source Function Solar Limb Geiger Counter 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Hearn, A.G.: 1963, Proc. Phys. Soc. 81, 648.ADSCrossRefGoogle Scholar
  2. Ivanov, V. V.: 1963, Soviet Astronomy-AJ 6, 793.ADSGoogle Scholar
  3. Pecker, C. and Thomes, R.N.: 1963, Astrophys. J. 137, 967.ADSCrossRefzbMATHGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1965

Authors and Affiliations

  • R. O. Redman
    • 1
  • L. De Feiter
    • 2
  1. 1.University of CambridgeCambridgeUK
  2. 2.Sterrewacht ‘Sonnenborgh’UtrechtThe Netherlands

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