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• W3037233223 abstract "The weak collisionality typical of turbulence in many diffuse astrophysical plasmas invalidates an MHD description of the turbulent dynamics, motivating the development of a more comprehensive theory of kinetic turbulence. In particular, a kinetic approach is essential for the investigation of the physical mechanisms responsible for the dissipation of astrophysical turbulence and the resulting heating of the plasma. This chapter reviews the limitations of MHD turbulence theory and explains how kinetic considerations may be incorporated to obtain a kinetic theory for astrophysical plasma turbulence. Key questions about the nature of kinetic turbulence that drive current research efforts are identified. A comprehensive model of the kinetic turbulent cascade is presented, with a detailed discussion of each component of the model and a review of supporting and conflicting theoretical, numerical, and observational evidence." @default.
• W3037233223 created "2020-07-02" @default.
• W3037233223 creator A5057492150 @default.
• W3037233223 date "2015-02-13" @default.
• W3037233223 modified "2023-09-26" @default.
• W3037233223 title "Kinetic Turbulence" @default.
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• W3037233223 doi "https://doi.org/10.1007/978-3-662-44625-6__6" @default.
• W3037233223 hasPublicationYear "2015" @default.
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