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

  • Wolfgang Rammacher
Conference paper


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


Acoustic Wave Energy Flux Flux Tube Magnetic Flux Tube Photospheric Magnetic Field 
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  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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