Velocity-space diffusion of solar wind protons in oblique waves and weak turbulence
The fast solar wind is permeated by all kinds of plasma waves which have a broad range of wavelengths and occur on many different scales. Kinetically, a plasma wave induces ion-wave interactions which can within the quasi-linear theory be described as a diffusion process. The impact this diffusio...
Main Authors: | E. Marsch, S. Bourouaine |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2011-11-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/29/2089/2011/angeo-29-2089-2011.pdf |
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