Linear theory of rotating fluids using spherical harmonics part I: Steady flows

DOI10.1080/03091928708208811zbMath0634.76106OpenAlexW1983805589WikidataQ114640363 ScholiaQ114640363MaRDI QIDQ3773629

Michel Rieutord

Publication date: 1987

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

Full work available at URL: https://doi.org/10.1080/03091928708208811

zbMATH Keywords

spherical harmonicsrotating fluidsequatorial singularity of steady boundary layerssteady spin-up of a fluid

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Basic methods in fluid mechanics (76M99)

Related Items (7)

Convergence and round-off errors in a two-dimensional eigenvalue problem using spectral methods and Arnoldi-Chebyshev algorithm ⋮ Axisymmetric inertial modes in a spherical shell at low Ekman numbers ⋮ Stress-driven spin-down of a viscous fluid within a spherical shell ⋮ Inertial waves in a differentially rotating spherical shell ⋮ Viscous dissipation by tidally forced inertial modes in a rotating spherical shell ⋮ Internal shear layers in librating spherical shells: the case of periodic characteristic paths ⋮ Gravito-inertial waves in a differentially rotating spherical shell

Cites Work

• The almost-rigid rotation of viscous fluid between concentric spheres
• Quasi-steady flow of a rotating stratified fluid in a sphere
• Patterns of convection in spherical shells. Part 2
• On almost rigid rotations. Part 2
• On the lnviscid Theory of Rotating Fluids
• Spin-up of a strongly stratified fluid in a sphere
• Viscous incompressible flow between concentric rotating spheres. Part 1. Basic flow
• An equatorial boundary layer

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