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Results From Optical and UV Stellar Flare Spectroscopy

Published online by Cambridge University Press:  12 April 2016

Mark S. Giampapa
Mark S. Giampapa*
Affiliation:
Harvard-Smithsonian Center for Astrophysics

Abstract

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Optical and ultraviolet spectroscopy can enable the assessment of the physical conditions characterizing a stellar flare atmosphere and thereby potentially elucidate the possible radiative and hydrodynamic transport mechanisms operative during stellar flares. In this review, I present illustrative examples of the spectroscopic diagnostic techniques that can be applied to the analysis of stellar flare spectroscopic data and the resulting inferences concerning stellar flare properties for M dwarf flare events.

Type
Session II: Observed Activity in Red-Dwarfs
Information
International Astronomical Union Colloquium , Volume 71: Activity in Red-Dwarf Stars , 1983 , pp. 223 - 235
Copyright
Copyright © Reidel 1983

References

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