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...

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Bibliographic Details
Main Authors: E. Marsch, S. Bourouaine
Format: Article
Language:English
Published: Copernicus Publications 2011-11-01
Series:Annales Geophysicae
Online Access:https://www.ann-geophys.net/29/2089/2011/angeo-29-2089-2011.pdf

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