Solar Wind Electron Acceleration via Langmuir Turbulence
The solar wind electrons observed at 1 AU are characterized by velocity distribution functions (VDF) that deviate from the Maxwellian form in a high energy regime. Such a feature is often modeled by a kappa distribution. In the present paper a self-consistent theory of quiet-time solar wind electron...
| Main Authors: | , , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Chinese Geoscience Union
2013-01-01
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| Series: | Terrestrial, Atmospheric and Oceanic Sciences |
| Subjects: | |
| Online Access: |
http://tao.cgu.org.tw/images/attachments/v242p175.pdf
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