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- W1572254596 abstract "AbstractEmission from high-energy electrons and ions in normal stars is a complex phenomenon since it is related to: (1) the energy release and particle acceleration processes, (2) the structure of the ambient magnetic field, and (3) the structure of the ambient atmosphere of these stars. Energy release, heating and acceleration are processes that are not well understood yet, so theoretical estimates of the high-energy emission is bound to use “artificial” velocity distribution functions for the energetic particles. We review the flow of energy in normal stars, the fundamental emission and absorption processes for spontaneous and collective emission and apply our results on selective observations. Our goal is to derive from the observations and the physics of radiation processes the properties of high-energy particles.KeywordsEnergetic ParticlePlasma WaveConvection ZoneStellar AtmosphereLoss ConeThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
- W1572254596 created "2016-06-24" @default.
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- W1572254596 date "1993-01-01" @default.
- W1572254596 modified "2023-09-27" @default.
- W1572254596 title "High energy emission from normal stars" @default.
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- W1572254596 doi "https://doi.org/10.1007/3-540-56874-3_3" @default.
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