2008
DOI: 10.1063/1.2839767
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Turbulent transport coefficients and residual energy in mean-field dynamo theory

Abstract: The turbulent electromotive force in the mean-field equation needs to be modeled to predict a large-scale magnetic field in magnetohydrodynamic turbulence at high Reynolds number. Using a statistical theory for inhomogeneous turbulence, model expressions for transport coefficients appearing in the turbulent electromotive force are derived including the α coefficient and the turbulent diffusivity. In particular, as one of the dynamo effects, the pumping effect is investigated and a model expression for the pump… Show more

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Cited by 7 publications
(10 citation statements)
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“…This implies that the magnetic fluctuation effect in the turbulent magnetic diffusivity may be suppressed due to the magnetic pressure, in particular in the case of incompressible MHD flow. This result is consistent with the traditional mean-field theories (Ra¨dler et al 2003, Brandenburg and Subramanian 2005, Ra¨dler and Rheinhardt 2007, Hamba and Sato 2008. …”
Section: 31supporting
confidence: 92%
See 2 more Smart Citations
“…This implies that the magnetic fluctuation effect in the turbulent magnetic diffusivity may be suppressed due to the magnetic pressure, in particular in the case of incompressible MHD flow. This result is consistent with the traditional mean-field theories (Ra¨dler et al 2003, Brandenburg and Subramanian 2005, Ra¨dler and Rheinhardt 2007, Hamba and Sato 2008. …”
Section: 31supporting
confidence: 92%
“…Actually higher-order contributions in the TSDIA were examined without resorting to the Elsasser formulation. It was found that the magnetic fluctuation contribution is canceled by the higher-order contributions (Hamba and Sato 2008). However, it is also probable that, if we proceed to further higher-order 130 N.…”
Section: Reynolds Stress and Turbulent Electromotive Forcementioning
confidence: 93%
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“…TSDIA is inconsistent with some classes of coordinate transformations. At least it has been pointed out so far that TSDIA results do not transform in a correct way under the time-dependent rotation [25]. More general criticism may be made from the view point of the covariance principle [26][27][28].…”
Section: Introductionmentioning
confidence: 99%
“…direct derivations of mean-vorticity effects in the vortex and MHD dynamos are actually avoided but instead are estimated so that the transformation rule Ω → Ω + 2ω p holds. Regarding the MHD dynamo, Ref [25]. has carefully pointed out the breaking of Euclidean invariance and made theoretical improvements by employing the corotational derivative instead of non-covariant Lagrangian derivative (see Eqs.…”
mentioning
confidence: 99%