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Discussion on Line Formation and Photospheric Structure

  • A. Unsöld
  • Wasaburo Unno
  • Yasumasa Yamashita
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 2)

Abstract

Areas on the photometric tracing enclosed by line profiles and an artificially truncated continuous level is studied. With these areas (fictitious equivalent widths), fictitious curves of growth can be constructed either theoretically or empirically. From the vertical and the horizontal shift between the theoretical and empirical curves, the Doppler width and the population of atoms are estimated for each truncated continuous level. Thus, the depth dependence of the Doppler width can be obtained empirically. For the solar photosphere, the result shows good agreement with the earlier determination by Unno.

Keywords

Line Profile Equivalent Width Line Formation Horizontal Shift Depth Dependence 
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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Copyright information

© Springer Science+Business Media Dordrecht 1965

Authors and Affiliations

  • A. Unsöld
    • 1
  • Wasaburo Unno
  • Yasumasa Yamashita
    • 2
  1. 1.University of KielKielGermany
  2. 2.Department of AstronomyUniversity of TokyoTokyoJapan

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