Linear theory of compressible convection in rapidly rotating spherical shells, using the anelastic approximation

DOI10.1017/S0022112009007253zbMath1183.76713OpenAlexW1984727491MaRDI QIDQ3550344

R. H. Mitchell, Chris A. Jones, K. M. Kuzanyan

Publication date: 31 March 2010

Published in: Journal of Fluid Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1017/s0022112009007253

Mathematics Subject Classification ID

Related Items (12)

Onset of rotating and non-rotating convection in compressible and anelastic ideal gases ⋮ The onset of strongly localized thermal convection in rotating spherical shells ⋮ Validity of sound-proof approaches in rapidly-rotating compressible convection: marginal stability versus turbulence ⋮ Quasi-geostrophic approximation of anelastic convection ⋮ Self-adjointness of sound-proof models for magnetic buoyancy ⋮ Stress-driven spin-down of a viscous fluid within a spherical shell ⋮ Radius ratio dependency of the instability of fully compressible convection in rapidly rotating spherical shells ⋮ Oscillatory convection and limitations of the Boussinesq approximation ⋮ Rigorous entropy formulation of the anelastic liquid equations in an ideal gas ⋮ Onset of fully compressible convection in a rapidly rotating spherical shell ⋮ Large-scale convective dynamos in a stratified rotating plane layer ⋮ The effect of stratification and compressibility on anelastic convection in a rotating plane layer

Cites Work

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• The quasi-geostrophic model for rapidly rotating spherical convection outside the tangent cylinder
• On the thermal instability of a rotating-fluid sphere containing heat sources
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