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Mesoturbulence in the Solar Atmosphere

  • R. I. Kostik
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 96)

Abstract

Solar spectral lines are observed to be broader and stronger than expected from purely thermal and pressure broadening. Classically, the broadening and strengthening are attributed to a macro- and microvelocity field. Such separation of the motions, however, does not take into account the physical nature of the turbulence and has a formal character.

Keywords

Central Intensity Correlation Length Solar Phys Solar Atmosphere Astronomical Observatory 
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.

References

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Copyright information

© D. Reidel Publishing Company 1982

Authors and Affiliations

  • R. I. Kostik
    • 1
  1. 1.Main Astronomical Observatory of the Ukrainian Academy of SciencesKiev-127USSR

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