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- W1615693430 abstract "The velocity distribution functions (VDFs) of electrons as measured in the solar wind show pronounced deviations from a Maxwellian. They seem to be composed of a thermal core and energetic tails, called halo. These VDFs can be fitted very well by kappa distributions. The formation of the energetic tails in the corona or in the solar wind is investigated. The relaxation of a kappa distribution under the influence of Coulomb collisions in the coronal plasma is calculated. This allows an estimation if the energetic tails of the VDFs can be formed in the corona. Resonant interaction between the electrons and electron cyclotron waves is suggested as a mechanism for the generation of the energetic tails. A kinetic model for electrons is presented. Coulomb collisions and wave‐particle interactions are considered. With this model, electron VDFs can be calculated from the transition region up into the solar wind." @default.
- W1615693430 created "2016-06-24" @default.
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- W1615693430 date "2003-01-01" @default.
- W1615693430 modified "2023-09-27" @default.
- W1615693430 title "Kinetics of Electrons in the Corona and Solar Wind" @default.
- W1615693430 doi "https://doi.org/10.1063/1.1618634" @default.
- W1615693430 hasPublicationYear "2003" @default.
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