Minimal tau approximation and simulations of the alpha effect
arXiv:astro-ph/0504222 · doi:10.1051/0004-6361:20053221
Abstract
The validity of a closure called the minimal tau approximation (MTA), is tested in the context of dynamo theory, wherein triple correlations are assumed to provide relaxation of the turbulent electromotive force. Under MTA, the alpha effect in mean field dynamo theory becomes proportional to a relaxation time scale multiplied by the difference between kinetic and current helicities. It is shown that the value of the relaxation time is positive and, in units of the turnover time at the forcing wavenumber, it is of the order of unity. It is quenched by the magnetic field -- roughly independently of the magnetic Reynolds number. However, this independence becomes uncertain at large magnetic Reynolds number. Kinetic and current helicities are shown to be dominated by large scale properties of the flow.
11 pages, 12 figures, accepted by A&A
References in corpus (5)
- The case for a distributed solar dynamo shaped by near-surface shear
- Simulations of nonhelical hydromagnetic turbulence
- Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations
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- Shear-current effect in a turbulent convection with a large-scale shear
- Kinetic and magnetic alpha effects in nonlinear dynamo theory
- Mean-field dynamo in a turbulence with shear and kinetic helicity fluctuations
- Simulations of the anisotropic kinetic and magnetic alpha effects
- Lambda-effect from forced turbulence simulations
- Local models of stellar convection III: The Strouhal number
- Nonlinear turbulent magnetic diffusion and effective drift velocity of large-scale magnetic field in a two-dimensional magnetohydrodynamic turbulence