Abstract
When coupled with a realistic acceleration model, the radiative signature of flare events in late-type stars is capable of giving additional, and more accurate, information concerning the nature of the accelerating regions than when the radiative signature is used alone. Here we consider the second-order Fermi, or stochastic acceleration mechanism.
The National Center for Atmospheric Research is sponsored by the National Science Foundation.
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© 1985 D. Reidel Publishing Company
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Bogdan, T.J., Schlickeiser, R. (1985). Stochastic Electron Acceleration in Stellar Coronae. In: Hjellming, R.M., Gibson, D.M. (eds) Radio Stars. Astrophysics and Space Science Library, vol 116. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5420-5_2
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DOI: https://doi.org/10.1007/978-94-009-5420-5_2
Publisher Name: Springer, Dordrecht
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