Chromospheric/Coronal Emission Correlations in ‘Quiescent’ and Eruptive Phenomena in M-Dwarf Stars
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.
KeywordsCoronal Heating Tangential Discontinuity Surface Magnetic Field Flare Star Solar Vicinity
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