Differential rotation driven by convection in a rapidly rotating annulus
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Publication:4747818
DOI10.1080/03091928208209005zbMath0508.76098OpenAlexW2009137281WikidataQ114640691 ScholiaQ114640691MaRDI QIDQ4747818
L. L. Hood, Friedrich H. Busse
Publication date: 1982
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091928208209005
differential rotationcentrifugally driven thermal convectioncurvature of conical surfacesdirection of mean flowgeneration of mean zonal flowrotating annulus heated from outside and cooled from within
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Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field ⋮ Reynolds stresses and mean fields generated by pure waves: applications to shear flows and convection in a rotating shell ⋮ Linear theory of compressible convection in rapidly rotating spherical shells, using the anelastic approximation ⋮ Convective flows in rapidly rotating spheres and their dynamo action ⋮ Subcritical convection of liquid metals in a rotating sphere using a quasi-geostrophic model ⋮ A model of mean zonal flows in the major planets ⋮ Physical interpretation of spiralling-columnar convection in a rapidly rotating annulus with radial propagation properties of Rossby waves ⋮ Numerical simulations of thermal convection in a rotating spherical fluid shell at high Taylor and Rayleigh numbers ⋮ Onset of fully compressible convection in a rapidly rotating spherical shell ⋮ Generation of mean flows by thermal convection
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