14–18 Feb 2011
Wenner Gren Center
Europe/Stockholm timezone

Compressibility effects on turbulent MHD and passive scalar transport

16 Feb 2011, 14:30
30m
Wenner-Gren Center, floor 7, Hörsalen (Wenner Gren Center)

Wenner-Gren Center, floor 7, Hörsalen

Wenner Gren Center

Sveavägen 164 SE-113 46 Stockholm Sweden

Speaker

Prof. Nathan Kleeorin

Description

The effects of compressibility (finite Mach number effect) and stratification of turbulent fluid flow on mean-field transport coefficients of magnetic field and passive scalar (number density of particles and temperature field) are studied for small and large magnetic Reynolds numbers (or small and large Peclet and Schmidt numbers) using correspondingly the quasi-linear approach and the spectral tau-approach. For small magnetic Reynolds numbers (or small Peclet numbers) the turbulent diffusion coefficient of both, magnetic and passive scalar fields coincide and decrease with increase of the degree of compressibility of turbulent velocity field (defined as the ratio of the mean square of divergence of velocity fluctuations to the mean square of curl of turbulent velocity field). At some value of the degree of compressibility of turbulent velocity field, the turbulent diffusion coefficient can be negative, but the total diffusion coefficient (molecular + turbulent) is always positive. For large magnetic Reynolds numbers (or large Peclet numbers) the compressibility of fluid flow reduces the turbulent diffusion coefficient, but it is always positive. On the other hand, the compressibility of an inhomogeneous turbulence causes the pumping velocity of the passive scalar in the direction of the gradient of the turbulence intensity, while the density stratification results in a counter gradient pumping velocity. Final effect of the gradient or the counter gradient transport depends on the value of the Mach number. The pumping velocity of the magnetic field is always counter gradient, and for small magnetic Reynolds numbers it is standard (determined by the gradient of the turbulent magnetic diffusion), while for large magnetic Reynolds numbers this velocity can increase with compressibility. The comparison with DNS results are also discussed.

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