Stellar flare statistics - Physical consequences

Details Stellar flare statistics - Physical consequences Stellar flare statistics - Physical consequences

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..375s&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Astronomy and Astrophysics

Astronomy

35

Energy Spectra, Statistical Correlation, Stellar Flares, Balmer Series, Decay Rates, Red Dwarf Stars, X Ray Astronomy

Scientific paper

The observational data make it possible to establish clear statistical correlations between different parameters of stellar flare activity and the characteristics of quiet stars. These relations are: (1) between energies and frequencies of flares on stars of different luminosities; (2) between total radiation energies of flares and quiet stars both in X-ray and Balmer emission lines; and (3) between flare decay rates just after the maxima and flare luminosities at maxima.

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