Nonlinear shear-current dynamo and magnetic helicity transport in sheared turbulence
arXiv:astro-ph/0609256 · doi:10.1080/03091920601004248
Abstract
The nonlinear mean-field dynamo due to a shear-current effect in a nonhelical homogeneous turbulence with a mean velocity shear is discussed. The transport of magnetic helicity as a dynamical nonlinearity is taken into account. The shear-current effect is associated with the term in the mean electromotive force, where is the mean vorticity due to the large-scale shear motions and is the mean electric current. This effect causes the generation of large-scale magnetic field in a turbulence with large hydrodynamic and magnetic Reynolds numbers. The dynamo action due to the shear-current effect depends on the spatial scaling of the correlation time of the background turbulence, where is the wave number. For Kolmogorov scaling, , the dynamo instability occurs, while when (small hydrodynamic and magnetic Reynolds numbers) there is no the dynamo action in a sheared nonhelical turbulence. The magnetic helicity flux strongly affects the magnetic field dynamics in the nonlinear stage of the dynamo action. Numerical solutions of the nonlinear mean-field dynamo equations which take into account the shear-current effect, show that if the magnetic helicity flux is not small, the saturated level of the mean magnetic field is of the order of the equipartition field determined by the turbulent kinetic energy. Turbulence with a large-scale velocity shear is a universal feature in astrophysics, and the obtained results can be important for elucidation of origin of the large-scale magnetic fields in astrophysical sheared turbulence.
13 pages, 13 figures, REVTEX4, Geophysical and Astrophysical Fluid Dynamics, in press
References in corpus (5)
- The case for a distributed solar dynamo shaped by near-surface shear
- Strong mean field dynamos require supercritical helicity fluxes
- Do mean-field dynamos in nonrotating turbulent shear-flows exist?
- The problem of small and large scale fields in the solar dynamo
- New mechanism of generation of large-scale magnetic fields in merging protogalactic and protostellar clouds
Cited by in corpus (7)
- Magnetic fluctuations and formation of large-scale inhomogeneous magnetic structures in a turbulent convection
- Large-scale instability in a sheared nonhelical turbulence: formation of vortical structures
- Shear-current effect in a turbulent convection with a large-scale shear
- Mean-field dynamo in a turbulence with shear and kinetic helicity fluctuations
- Alpha-effect dynamos with zero kinetic helicity
- Nonlinear turbulent magnetic diffusion and effective drift velocity of large-scale magnetic field in a two-dimensional magnetohydrodynamic turbulence
- New mechanism of generation of large-scale magnetic field in a sheared turbulent plasma