Fully developed MHD turbulence near critical magnetic Reynolds number
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Publication:3898253
DOI10.1017/S002211208100298XzbMath0451.76089OpenAlexW1984105248MaRDI QIDQ3898253
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Publication date: 1981
Published in: Journal of Fluid Mechanics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1017/s002211208100298x
Related Items (8)
An asymptotic analysis of a small-scale dynamo in a mirror-asymmetric random velocity field ⋮ THE MAGNETIZED UNIVERSE ⋮ A dynamo theorem ⋮ Turbulent magnetic field amplification from the smallest to the largest magnetic Prandtl numbers ⋮ Turbulence theories and statistical closure approaches ⋮ The macroscopic magnetohydrodynamics of inhomogeneously turbulent cosmic plasmas ⋮ Fully developed turbulent dynamo at low magnetic Prandtl numbers ⋮ Fully developed turbulent dynamo at low magnetic Prandtl numbers
Cites Work
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- A refinement of previous hypotheses concerning the local structure of turbulence in a viscous incompressible fluid at high Reynolds number
- Progress in the development of a Reynolds-stress turbulence closure
- Strong MHD helical turbulence and the nonlinear dynamo effect
- A simple dynamical model of intermittent fully developed turbulence
- Numerical simulation of helical magnetohydrodynamic turbulence
- Formulation of the Theory of Turbulence
- Growth of Turbulent Magnetic Fields
- Analytical theories of turbulence
- On the spontaneous magnetic field in a conducting liquid in turbulent motion
- Cosmic Radiation and Cosmic Magnetic Fields. II. Origin of Cosmic Magnetic Fields
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