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Balmer and soft X-ray emission from solar and stellar flares
Published online by Cambridge University Press: 23 September 2016
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
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- Copyright
- Copyright © Kluwer 1990
References
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