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Updated: Jul 11, 2026

06:42
Magnetically Induced Rotating Rayleigh-Taylor Instability
Published on: March 3, 2017
Transport in two-fluid magnetohydrodynamic turbulence
1Department of Applied Mathematics, University of Sheffield, Sheffield, S3 7RH, United Kingdom.
Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|October 13, 2007
Summary
This study introduces a theory for turbulent transport in two-fluid reduced magnetohydrodynamics (MHD). Kinetic Alfven waves weaken magnetic field quenching, reducing turbulent magnetic diffusivity.
Area of Science:
- Plasma Physics
- Fluid Dynamics
- Magnetohydrodynamics (MHD)
Background:
- Turbulent transport of magnetic flux and momentum is crucial in plasma physics.
- Single-fluid reduced MHD models often overestimate the quenching of magnetic fields.
Purpose of the Study:
- To develop a theory for transport in two-fluid 3D reduced MHD turbulence.
- To investigate the role of kinetic Alfven waves and shear flows on turbulent transport.
Main Methods:
- Theoretical modeling of two-fluid reduced MHD turbulence.
- Consistent inclusion of shear flows and magnetic fields.
- Analysis of kinetic Alfven wave and drift wave effects.
Main Results:
- Kinetic Alfven waves weaken turbulent transport quenching of strong magnetic fields.
- Turbulent magnetic diffusivity is proportional to (eta/Omega)^(1/3)B(0)^(-2).
- Momentum transport is diffusive with enhanced eddy viscosity compared to single-fluid MHD.
Conclusions:
- Two-fluid effects, particularly kinetic Alfven waves, are essential for accurate modeling of turbulent transport.
- The findings have implications for understanding shear flow instabilities in magnetized plasmas.
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