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Physical Conditions in Solar Coronal Holes on the Base of Non-LTE Calculations

  • E. Malanushenko
  • E. Baranovsky
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 259)

Abstract

We show that the intensity variations of the He I 10830 Å and the H Lyα lines which are observed in coronal holes and quiet regions can be explained by the model variations in the upper chromosphere.

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Copyright information

© Springer Science+Business Media Dordrecht 2001

Authors and Affiliations

  • E. Malanushenko
    • 1
  • E. Baranovsky
    • 1
  1. 1.Crimean Astrophysical ObservatoryCrimeaUkraine

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