Two-dimensional state in driven magnetohydrodynamic turbulence
- Space Science Center, University of New Hampshire, Durham, New Hampshire 03824 (United States)
- Universite Paris-Sud, Institut d'Astrophysique Spatiale, bat. 121, F-91405 Orsay (France)
The dynamics of the two-dimensional (2D) state in driven three-dimensional (3D) incompressible magnetohydrodynamic turbulence is investigated through high-resolution direct numerical simulations and in the presence of an external magnetic field at various intensities. For such a flow the 2D state (or slow mode) and the 3D modes correspond, respectively, to spectral fluctuations in the plane k{sub ||}=0 and in the area k{sub ||}>0. It is shown that if initially the 2D state is set to zero it becomes nonnegligible in few turnover times, particularly when the external magnetic field is strong. The maintenance of a large-scale driving leads to a break for the energy spectra of 3D modes; when the driving is stopped, the previous break is removed and a decay phase emerges with Alfvenic fluctuations. For a strong external magnetic field the energy at large perpendicular scales lies mainly in the 2D state, and in all situations a pinning effect is observed at small scales.
- OSTI ID:
- 21560034
- Journal Information:
- Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print), Vol. 83, Issue 2; Other Information: DOI: 10.1103/PhysRevE.83.026405; (c) 2011 American Institute of Physics; ISSN 1539-3755
- Country of Publication:
- United States
- Language:
- English
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GENERAL PHYSICS
ALFVEN WAVES
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DECAY
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RESOLUTION
THREE-DIMENSIONAL CALCULATIONS
TURBULENCE
TWO-DIMENSIONAL CALCULATIONS
FLUID MECHANICS
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HYDROMAGNETIC WAVES
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SPECTRA
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