Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2011-05-29
Phys. Rev. E 84, 056314 (2011)
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
12 pages, 9 figures, REVTEX4-1, revised version
Scientific paper
10.1103/PhysRevE.84.056314
Using different analytical methods (the quasi-linear approach, the path-integral technique and tau-relaxation approximation) we develop a comprehensive mean-field theory for a pumping effect of the mean magnetic field in homogeneous non-rotating helical turbulence with imposed large-scale shear. The effective pumping velocity is proportional to the product of alpha effect and large-scale vorticity associated with the shear, and causes a separation of the toroidal and poloidal components of the mean magnetic field along the direction of the mean vorticity. We also perform direct numerical simulations of sheared turbulence in different ranges of hydrodynamic and magnetic Reynolds numbers and use a kinematic test-field method to determine the effective pumping velocity. The results of the numerical simulations are in agreement with the theoretical predictions.
Brandenburg Axel
Käpylä Petri
Kleeorin Nathan
Rogachevskii Igor
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