Mean-field diffusivities in passive scalar and magnetic transport in irrotational flows

Karl-Heinz Rädler, Axel Brandenburg, Fabio Del Sordo, and Matthias Rheinhardt
Phys. Rev. E 84, 046321 – Published 25 October 2011

Abstract

Certain aspects of the mean-field theory of turbulent passive scalar transport and of mean-field electrodynamics are considered with particular emphasis on aspects of compressible fluids. It is demonstrated that the total mean-field diffusivity for passive scalar transport in a compressible flow may well be smaller than the molecular diffusivity. This is in full analogy to an old finding regarding the magnetic mean-field diffusivity in an electrically conducting turbulently moving compressible fluid. These phenomena occur if the irrotational part of the motion dominates the vortical part, the Péclet or magnetic Reynolds number is not too large, and, in addition, the variation of the flow pattern is slow. For both the passive scalar and the magnetic cases several further analytical results on mean-field diffusivities and related quantities found within the second-order correlation approximation are presented, as well as numerical results obtained by the test-field method, which applies independently of this approximation. Particular attention is paid to nonlocal and noninstantaneous connections between the turbulence-caused terms and the mean fields. Two examples of irrotational flows, in which interesting phenomena in the above sense occur, are investigated in detail. In particular, it is demonstrated that the decay of a mean scalar in a compressible fluid under the influence of these flows can be much slower than without any flow, and can be strongly influenced by the so-called memory effect, that is, the fact that the relevant mean-field coefficients depend on the decay rates themselves.

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  • Received 8 April 2011

DOI:https://doi.org/10.1103/PhysRevE.84.046321

©2011 American Physical Society

Authors & Affiliations

Karl-Heinz Rädler1,2,3,*, Axel Brandenburg2,4,3, Fabio Del Sordo2,4, and Matthias Rheinhardt2

  • 1Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
  • 2NORDITA, AlbaNova University Center, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden
  • 3Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA
  • 4Department of Astronomy, Stockholm University, SE-10691 Stockholm, Sweden

  • *khraedler@arcor.de

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Issue

Vol. 84, Iss. 4 — October 2011

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