The influence of a mean magnetic field on three-dimensional magnetohydrodynamic turbulence
- 10 December 1994
- journal article
- research article
- Published by Cambridge University Press (CUP) in Journal of Fluid Mechanics
- Vol. 280, 95-117
- https://doi.org/10.1017/s0022112094002867
Abstract
Building on results from two-dimensional magnetohydrodynamic (MHD) turbulence (Shebalin, Matthaeus & Montgomery 1983), the development of anisotropic states from initially isotropic ones is investigated numerically for fully three-dimensional incompressible MHD turbulence. It is found that when an external d.c. magnetic field (B0) is imposed on viscous and resistive MHD systems, excitations are preferentially transferred to modes with wavevectors perpendicular to B0). The anisotropy increases with increasing mechanical and magnetic Reynolds numbers, and also with increasing wavenumber. The tendency of B0 to inhibit development of turbulence is also examined.Keywords
This publication has 22 references indexed in Scilit:
- An analysis of subgrid-scale interactions in numerically simulated isotropic turbulencePhysics of Fluids A: Fluid Dynamics, 1993
- Nearly incompressible fluids. II: Magnetohydrodynamics, turbulence, and wavesPhysics of Fluids A: Fluid Dynamics, 1993
- Statistical properties of ideal three-dimensional magnetohydrodynamicsPhysics of Fluids B: Plasma Physics, 1990
- Dynamics of decaying two-dimensional magnetohydrodynamic turbulencePhysics of Fluids B: Plasma Physics, 1989
- Turbulent magnetic reconnectionPhysics of Fluids, 1986
- Viscosity and the Chew-Goldberger-Low equations in the solar coronaThe Astrophysical Journal, 1986
- Growth of correlations in magnetohydrodynamic turbulencePhysical Review A, 1986
- Forced magnetohydrodynamic turbulence in a uniform external magnetic fieldPhysics of Fluids, 1985
- Fully Developed Anisotropic Hydromagnetic Turbulence in Interplanetary SpacePhysical Review Letters, 1980
- Two-dimensional turbulenceReports on Progress in Physics, 1980