A model of mean zonal flows in the major planets
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Publication:3042681
DOI10.1080/03091928308221746zbMath0527.76018OpenAlexW1984346013WikidataQ114640572 ScholiaQ114640572MaRDI QIDQ3042681
Publication date: 1983
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091928308221746
curvaturePrandtl numberinhomogeneityzonal flowsinertial wavesEkman numberrotation effectsannular flows past Jupiter and Saturnband structure of atmosphere of major planetsconvection mechanism
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Cites Work
- An experimental and theoretical investigation of the onset of convection in rotating spherical shells
- On the propagation and stability of wave motions in rapidly rotating spherical shells: I. The non-magnetic case
- On diffusive instabilities of a rapidly rotating electrically conducting layer of compressible fluid of varying depth
- Convection in rapidly rotating spherical fluid shells
- On the Finite amplitude thermal instability of a rapidly rotating fluid sphere
- Differential rotation driven by convection in a rapidly rotating annulus
- On the thermal instability of a rotating-fluid sphere containing heat sources
- Thermal instabilities in rapidly rotating systems
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