Astrophysical Hydromagnetic Turbulence
作者： A. Brandenburg , A. Lazarian
DOI: 10.1007/S11214-013-0009-3
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摘要: Recent progress in astrophysical hydromagnetic turbulence is being reviewed. The physical ideas behind the now widely accepted Goldreich–Sridhar model and its extension to compressible magnetohydrodynamic are introduced. Implications for cosmic ray diffusion acceleration discussed. Dynamo-generated magnetic fields with without helicity contrasted against each other. Certain turbulent transport processes modified often suppressed by anisotropy inhomogeneities of turbulence, while others produced such properties, which can lead new large-scale instabilities medium. Applications various systems considered.
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