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Stellar Flare Statistics - Physical Consequences

Published online by Cambridge University Press:  12 April 2016

N. I. Shakhovskaya
N. I. Shakhovskaya*
Affiliation:
Crimean Astrophysical Observatory, 334413 p/o Nauchny, Crimea, U.S.S.R.

Abstract

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The observational data permit us to establish clear statistical correlations between different parameters of stellar flare activity and the characteristics of quiet stars. These relations are:

  1. (i) between energies and frequencies of flares on stars of different luminosities;

  2. (ii) between total radiation energies of flares and quiet stars both in X-ray and Balmer emission lines;

  3. (iii) between flare decay rates just after the maxima and flare luminosities at maxima.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 104 , Issue 1: Solar and Stellar Flares , 1989 , pp. 375 - 386
Copyright
Copyright © Kluwer 1989

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