Dynamics of decaying two-dimensional magnetohydrodynamic turbulence
- Max-Planck-Institut fur Plasmaphysik, EURATOM Association, 8046 Garching bei Munchen, Federal Republic of Germany (DE)
High-resolution numerical studies of decaying two-dimensional magnetohydrodynamic turbulence were performed with up to 1024{sup 2} collocation points in general periodic systems using various initial states, but restricting consideration to weak velocity-magnetic field correlation {rho}. The global evolution is self-similar with constant kinetic to magnetic energy ratio {ital E}{sup {ital V}}/{ital E}{sup {ital M}}, macro- and microscale Reynolds numbers, and correlation {rho}, while the total energy decays as {ital E}({ital t}){proportional to}({ital t}+{ital t}{sub 0}){sup {minus}1}. As in three dimensions, dissipative small-scale turbulence adjusts in such a way as to make the energy dissipation rate {epsilon} independent of the collisional dissipation coefficients. Normalized energy spectra are also invariant. The spectral index in the inertial range is, in general, close to 3/2 in agreement with Kraichnan's Alfven wave argument {ital E}{sub {ital k}} ={ital DB}{sup 1/2}{epsilon}{sup 1/2}{ital k}{sup {minus}3/2}, {ital B}=({ital E}{sup {ital M}}){sup 1/2}, {ital D}{congruent} 1.8{plus minus}0.2, but may be close to 5/3 in transient states, in which turbulence is concentrated in regions of weak magnetic field. In the dissipation range, intermittency gives rise to a modified dissipation scale {ital l}{sub eff} =({ital l}{sup 2}{lambda}){sup 1/3}, with {ital l}=Kolmogorov scale and {lambda}=Taylor microscale. This reflects the intermittency of the dissipation process, which is consistent with the picture of current microsheets of thickness {ital l} and width and spacing {lambda}.
- OSTI ID:
- 5336612
- Journal Information:
- Physics of Fluids B: Plasma Physics; (USA), Vol. 1:10; ISSN 0899-8221
- Country of Publication:
- United States
- Language:
- English
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SUPERCONDUCTIVITY AND SUPERFLUIDITY
FLUIDS
TURBULENCE
COLLISIONAL PLASMA
ENERGY LOSSES
ENERGY SPECTRA
INVARIANCE PRINCIPLES
MAGNETIC FIELDS
MAGNETOHYDRODYNAMICS
NUMERICAL SOLUTION
OSCILLATION MODES
RESOLUTION
REYNOLDS NUMBER
TRANSIENTS
TWO-DIMENSIONAL CALCULATIONS
FLUID MECHANICS
HYDRODYNAMICS
LOSSES
MECHANICS
PLASMA
SPECTRA
640410* - Fluid Physics- General Fluid Dynamics