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Diffusion and transport of a magnetic field in a turbulent medium with helicity
Authors:N A Silant’ev
Institution:(1) Central Astronomical Observatory, Russian Academy of Sciences, 196140 St. Petersburg, Russia;(2) Instituto National de Astrofisica, Optica y Electronica, Puebla, Mexico
Abstract:An analysis is made of the relation between accurate formulas for the coefficients of turbulent diffusion D T and the alpha effect α T for a magnetic field in the Lagrange and Euler representations. It is shown that the quadratic term with respect to α T in the diffusion coefficient derived by Moffatt and Kraichnan is incorrect and should be dropped. First, a numerical solution of the nonlinear equation (DIA equation) for the Green function is presented, describing the transport of a magnetic field for the case of incompressible, uniform, isotropic, steady-state turbulence possessing helicity. These solutions are used to calculate the steady-state coefficients D T and α T for various values of the parameters ξ 0=u 0 σ 0/R 0, a=H 0/u 0 2 p 0, σ 0/σ 1, and R 0/R 1, where u 0, σ 0, and R 0 are the characteristic velocity, lifetime, and scale of the turbulent pulsations, and H 0, σ 1, and R 1 are similar values describing the helicity of the medium h(1,2)=〈u(1)· (∇×u(2))〉, and the parameter α characterizes the degree of helicity. The DIA values of D T and α T and the self-consistent values of these quantities calculated using the Green tensor in the diffusion approximation are in qualitative agreement. It is shown that the coefficient of turbulent diffusion is always positive for all the types of turbulence studied. Nonsteady-state values of D T(t) and α T(t) calculated by a self-consistent method are given. Zh. éksp. Teor. Fiz. 112, 1312–1331 (October 1997)
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