Magnetic dynamo action in two-dimensional turbulent magneto-hydrodynamics
Two-dimensional magnetohydrodynamic turbulence is explored by means of numerical simulation. Previous analytical theory, based on non-dissipative constants of the motion in a truncated Fourier representation, is verified by following the evolution of highly non-equilibrium initial conditions numerically. Dynamo action (conversion of a significant fraction of turbulent kinetic energy into long-wavelength magnetic field energy) is observed. It is conjectured that in the presence of dissipation and external forcing, a dual cascade will be observed for zero-helicity situations. Energy will cascade to higher wave numbers simultaneously with a cascade of mean square vector potential to lower wave numbers, leading to an omni-directional magnetic energy spectrum which varies as k/sup -1/3/ at lower wave numbers, simultaneously with a buildup of magnetic excitation at the lowest wave number of the system. Equipartition of kinetic and magnetic energies is expected at the highest wave numbers in the system.
- Research Organization:
- Univ. of Iowa, Iowa City (United States). Dept. of Physics and Astronomy; National Center for Atmospheric Research, Boulder, CO (USA)
- Sponsoring Organization:
- US Energy Research and Development Administration (ERDA)
- DOE Contract Number:
- E(11-1)-2059
- OSTI ID:
- 7130490
- Report Number(s):
- COO-2059-54
- Country of Publication:
- United States
- Language:
- English
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640430* - Fluid Physics- Magnetohydrodynamics