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 (17)
- The inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence
- The case for a distributed solar dynamo shaped by near-surface shear
- Simulations of nonhelical hydromagnetic turbulence
- Magnetic Helicity Conservation and Astrophysical Dynamos
- A New Dynamical Mean-Field Dynamo Theory and Closure Approach
- Dynamic nonlinearity in large scale dynamos with shear
- Electromotive Force and Large-Scale Magnetic Dynamo in a Turbulent Flow with a Mean Shear
- Nonlinear theory of a "shear-current" effect and mean-field magnetic dynamos
- Dynamical Quenching of the Dynamo
- Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations
- Nonlinear current helicity fluxes in turbulent dynamos and alpha quenching
- The Role of Magnetic Helicity Transport in Nonlinear Galactic Dynamos
- Coronal activity as a consequence of dynamos in astrophysical rotators
- Direct simulations of helical Hall-MHD turbulence and dynamo action
- Catastrophic alpha quenching alleviated by helicity flux and shear
- Magnetic helicity evolution in a periodic domain with imposed field
- Apparent suppression of turbulent magnetic dynamo action by a dc magnetic field
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- Galactic spiral patterns and dynamo action I: A new twist on magnetic arms
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- Mean--field electrodynamics: Critical analysis of various analytical approaches to the mean electromotive force
- Magnetoconvection and dynamo coefficients III: alpha-effect and magnetic pumping in the rapid rotation regime
- Turbulent dynamos with shear and fractional helicity
- The negative effective magnetic pressure in stratified forced turbulence
- Advances in theory and simulations of large-scale dynamos
- Large-scale instability in a sheared nonhelical turbulence: formation of vortical structures
- Shear-current effect in a turbulent convection with a large-scale shear
- Kinetic and magnetic alpha effects in nonlinear dynamo theory
- Traces of large-scale dynamo action in the kinematic stage
- The alpha effect with imposed and dynamo-generated magnetic fields
- Magnetic helicity and energy spectra of a solar active region
- Two-scale analysis of solar magnetic helicity
- Polarization of gravitational waves from helical MHD turbulent sources
- Scale-invariant helical magnetic field evolution and the duration of inflation
- Pumping velocity in homogeneous helical turbulence with shear
- Mean-field dynamo in a turbulence with shear and kinetic helicity fluctuations
- Open and closed boundaries in large-scale convective dynamos
- Evolution of Magnetic Helicity and Energy Spectra of Solar Active Regions
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- Galactic Spiral Patterns and Dynamo Action II: Asymptotic Solutions
- Hall cascade with fractional magnetic helicity in neutron star crusts
- Lambda-effect from forced turbulence simulations
- Simulations of the anisotropic kinetic and magnetic alpha effects
- Calibrating passive scalar transport in shear-flow turbulence
- The critical role of magnetic helicity in astrophysical large-scale dynamos
- Simulations of a Magnetic Fluctuation Driven Large Scale Dynamo and Comparison with a Two-scale Model
- Competition of rotation and stratification in flux concentrations
- Magnetic and rotational quenching of the effect
- On the resilience of helical magnetic fields to turbulent diffusion and the astrophysical implications
- Chiral magnetohydrodynamics with zero total chirality
- Turbulent magnetic helicity fluxes in solar convective zone
- Non-linear Galactic Dynamos and the Magnetic Rädler Effect
- Solar Kinetic Energy and Cross Helicity Spectra
- Derivation and precision of mean field electrodynamics with mesoscale fluctuations
- Laboratory Plasma Dynamos, Astrophysical Dynamos, and Magnetic Helicity Evolution
- Small-scale magnetic buoyancy and magnetic pumping effects in a turbulent convection
- EDGES signal in presence of magnetic fields
- High Reynolds number magnetohydrodynamic turbulence using a Lagrangian model
- Effect of heat flux on differential rotation in turbulent convection
- A global galactic dynamo with a corona constrained by relative helicity
- Experimental study of turbulent thermal diffusion of particles in an inhomogeneous forced convective turbulence
- A new constraint on mean-field galactic dynamo theory
- Local models of stellar convection III: The Strouhal number
- An advective solar-type dynamo without the alpha effect
- Kinetic helicity decay in linearly forced turbulence
- Mean-field closure parameters for passive scalar turbulence
- Negative Magnetic Diffusivity beta replacing alpha effect in Helical Dynamo
- Ribbons characterize magnetohydrodynamic magnetic fields better than lines: a lesson from dynamo theory
- Magnetic helicity in primordial and dynamo scenarios of galaxies
- Nonlinear turbulent magnetic diffusion and effective drift velocity of large-scale magnetic field in a two-dimensional magnetohydrodynamic turbulence
- Application of the electromotive force as a shock front indicator in the inner heliosphere
- New mechanism of generation of large-scale magnetic field in a sheared turbulent plasma
- Compressibility effects in a turbulent transport of temperature field
- Generation of a large-scale vorticity in a fast rotating density stratified turbulence or turbulent convection
- Analysis of the Effect of a Mean Velocity Field on Mean Field Dynamo
- Turbulent transport of radiation in the solar convective zone
- Resistive Scaling in the Magnetic Helicity-Driven Inverse Cascade