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Diffusion and dispersion in magnetohydrodynamic turbulence:: The influence of mean magnetic fields

期刊

ASTRONOMISCHE NACHRICHTEN
卷 329, 期 7, 页码 714-716

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WILEY-V C H VERLAG GMBH
DOI: 10.1002/asna.200811011

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diffusion; magnetohydrodynamics (MHD); turbulence

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The properties of magnetohydrodynamic (MHD) turbulence under the influence of a strong mean magnetic field are investigated from the Lagrangian viewpoint by tracking fluid particles in direct numerical simulations. The particle trajectories show characteristic bends near vortex sheets. A strong mean magnetic field leads to preferential diffusion parallel to the mean magnetic field. The two-particle relative dispersion process shows a dependence on the orientation of the initial separation vector. The relative dispersion is slowed down for initial separation vectors aligned with the mean magnetic field. (C) 2008 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

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