Turbulent thermal convection in the presence of rotation and a magnetic field: A heuristic theory

DOI10.1080/03091927908242681zbMath0434.76093OpenAlexW2093989665WikidataQ114640900 ScholiaQ114640900MaRDI QIDQ3873845

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Publication date: 1979

Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1080/03091927908242681

zbMATH Keywords

rotationmagnetic fieldheuristicturbulent thermal convectionanalytical resultsnon-linearitiesplanar geometryshear instabilitiesstellar and planetary dynamossuperadiabatic fluid

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar dynamics (85A05) Diffusion and convection (76R99) Geo-electricity and geomagnetism (86A25)

Related Items (5)

Approaching a realistic force balance in geodynamo simulations ⋮ Scaling regimes in spherical shell rotating convection ⋮ Anisotropic evolution of small isolated vortices within the core of the Earth ⋮ Force balance in rapidly rotating Rayleigh–Bénard convection ⋮ Large-scale vortices and zonal flows in spherical rotating convection

Cites Work

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• Stability of parallel flow in a parallel magnetic field at small magnetic Reynolds numbers
• Convection in rapidly rotating spherical fluid shells
• The onset of shear instability in stars
• Turbulent convection within rapidly rotating superadiabatic fluids with horizontal temperature gradients
• Heat transport by turbulent convection
• Stability of Hydromagnetic Kelvin-Helmholtz Discontinuity
• Hydromagnetic instability of a free shear layer at small magnetic Reynolds numbers
• Hydromagnetic convection in a rapidly rotating fluid layer
• Magnetohydrodynamics of the Earth's Core
• Turbulent Thermal Convection at Arbitrary Prandtl Number
• Transport of Heat and Matter by Convection in Stars
• The heat transport and spectrum of thermal turbulence

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