The macroscopic magnetohydrodynamics of inhomogeneously turbulent cosmic plasmas
DOI10.1080/03091928308209069zbMath0541.76146OpenAlexW1987827317WikidataQ114640598 ScholiaQ114640598MaRDI QIDQ3329112
L. L. Kichatinov, S. I. Vainshtein
Publication date: 1983
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091928308209069
magnetic forceinhomogeneous turbulencelarge-scale magnetic fieldmagnetic fluctuationsdiamagnetic effectdynamo problemaveraged fieldfield line distortioninteraction with the fluctuationsmagnetohydrodynamic turbulence at high magnetic Reynolds numbersOrszag schemesecond- order momentsself-reactionsmall-scale magnetic field helicity
Nonlinear effects in hydrodynamic stability (76E30) Magnetohydrodynamics and electrohydrodynamics (76W05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)
Related Items (8)
Cites Work
- Magnetic field transfer by two-dimensional convection and solar 'semi- dynamo'
- Fully developed MHD turbulence near critical magnetic Reynolds number
- Possibility of an inverse cascade of magnetic helicity in magnetohydrodynamic turbulence
- Strong MHD helical turbulence and the nonlinear dynamo effect
- Growth of Turbulent Magnetic Fields
- Analytical theories of turbulence
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