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Line Simulation of Solar Structures Permeated by Acoustic and MHD-Waves

  • Wolfgang Rammacher
Conference paper

Abstract

MgII-k and CaII-K-line-profiles generated by acoustic and MHD-waves of different periods and fixed energy flux are computed.

Keywords

Acoustic Wave Energy Flux Flux Tube Magnetic Flux Tube Photospheric Magnetic Field 
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. Ulmschneider, Kalkofen, Nowak, Bohn: 1977, Astron. Astrophys. 54, 61ADSGoogle Scholar
  2. Ulmschneider, Schmitz, Kalkofen, Bohn: 1978, Astron. Astrophys. 70, 487ADSGoogle Scholar
  3. Solanki, Roberts: 1989, in “The solar photosphere”, IAU- Symp. 132, Kluwer, Dordrecht (1989)Google Scholar

Copyright information

© Springer-Verlag Berlin Heidelberg 1991

Authors and Affiliations

  • Wolfgang Rammacher
    • 1
  1. 1.Institut für Theoretische AstrophysikUniversität HeidelbergHeidelberg 1Federal Republic of Germany

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