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Relationship between the Line Formation Depth and Stratification of Vector Magnetic Fields in the Solar Atmosphere

  • Z. Q. Qu
  • X. M. Gu
Part of the Astrophysics and Space Science Library book series (ASSL, volume 243)

Abstract

The relationship between the line formation depth obtained from contribution function and the stratification of vector magnetic field is discussed. It is argued that probing the stratification by employing several lines, to which one assigns formation heights, can be meaningless.

Key words

Line: formation Radiative transfer Solar magnetic fields 

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References

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Copyright information

© Springer Science+Business Media Dordrecht 1999

Authors and Affiliations

  • Z. Q. Qu
    • 1
  • X. M. Gu
    • 1
  1. 1.Yunnan Astronomical ObservatoryChinese Academy of SciencesKunmingP.R. China

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