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The Model of the Impulsive Phase of Stellar Flares

Published online by Cambridge University Press:  27 September 2017

V.P. Grinin  and
V.V. Sobolev
V.P. Grinin
Affiliation:
Crimean Astrophysical Observatory, 334413, p/o Nauchny, USSR
V.V. Sobolev
Affiliation:
Leningrad State University, 198904, St. Petergoff, USSR

Abstract

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The arguments in favour of that the primary heating of the gas at the impulsive phase of stellar flares is caused by charged particles of higher energies than in the solar flares are given. It is shown that the model of the deep heating by high energy protons (E ≃ 10 MeV) or electrons (E ≃ 100 keV) with taken into account of the radiative transfer in flare region explane the main properties of the optical continuum of the flare.

Type
Session III: Theory
Information
International Astronomical Union Colloquium , Volume 104 , Issue 2: Solar and Stellar Flares , 1989 , pp. 297 - 300
Copyright
Copyright © Kluwer 1989

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