Astrophysical gyrokinetics: Basic equations and linear theory

Magnetohydrodynamic (MHD) turbulence is encountered in a wide variety of astrophysical plasmas, including accretion disks, the solar wind, and the interstellar and intracluster medium. On small scales, this turbulence is often expected to consist of highly anisotropic fluctuations with frequencies s...

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Bibliografische gegevens
Hoofdauteurs: Howes, G, Cowley, S, Dorland, W, Hammett, G, Quataert, E, Schekochihin, A
Formaat: Journal article
Taal:English
Gepubliceerd in: 2006