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Chromospheric/Coronal Emission Correlations in ‘Quiescent’ and Eruptive Phenomena in M-Dwarf Stars

  • M. Mathioudakis
  • J. G. Doyle
Conference paper

Abstract

A power-law linear correlation between Hγ and soft X-ray emission is presented. It is remarkablo, that the relationship, Lx = 34 × L γ, holds over several orders of magnitude for both ‘quiescent’ and flare (solar and stellar) observations. The data are discussed in terms of microflaring.

Keywords

Coronal Heating Tangential Discontinuity Surface Magnetic Field Flare Star Solar Vicinity 
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

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Copyright information

© Springer-Verlag Berlin Heidelberg 1991

Authors and Affiliations

  • M. Mathioudakis
    • 1
  • J. G. Doyle
    • 1
  1. 1.Armagh ObservatoryArmaghN. Ireland

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