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Balmer and soft X-ray emission from solar and stellar flares

Published online by Cambridge University Press:  23 September 2016

C. J. Butler
C. J. Butler*
Affiliation:
Armagh Observatory, N. Ireland

Abstract

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Integrated soft X-ray (8-12A) fluxes for solar flares have been scaled to the equivalent EXOSAT fluxes using spectra obtained from a variety of rocket-based experiments. The data show good agreement with the soft X-ray - Hγ correlation established by Butler et al. (1988) for stellar flares and confirm the basic similarity, in this respect, of flares on the Sun to those on dMe stars.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 153 - 157
Copyright
Copyright © Kluwer 1990 

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