Character and stability of axisymmetric thermal convection in spheres and spherical shells

DOI10.1080/03091928308209038zbMath0519.76038OpenAlexW2080913678WikidataQ114640629 ScholiaQ114640629MaRDI QIDQ3669050

Abdelfattah Zebib, Gerald Schubert, James L. Dein, Ramesh C. Paliwal

Publication date: 1983

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

Full work available at URL: https://doi.org/10.1080/03091928308209038

zbMATH Keywords

spheresself-gravitatingheat transfer characteristics of non-self-adjoint systemsinfinite Prandtl number fluidsmodes of heatingnonlinear axisymmetric motionsthick spherical shells

Mathematics Subject Classification ID

Absolute and convective instability and stability in hydrodynamic stability (76E15) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (4)

Numerical simulations of mantle convection: Time-dependent, three-dimensional, compressible, spherical shell ⋮ Linear and weakly nonlinear variable viscosity convection in spherical shells ⋮ Three-dimensional convection in spherical shells ⋮ Weakly nonlinear mode interactions in spherical Rayleigh–Bénard convection

Cites Work

• Finite prandtl number convection in spherical shells
• Thermal convection of an internally heated infinite prandtl number fluid in a spherical shell
• Infinite Prandtl number thermal convection in a spherical shell
• Patterns of convection in spherical shells
• Axisymmetric convection in a rotating sphere. Part 1. Stress-free surface
• Convection due to internal heat sources
• Axisymmetric convection in a rotating sphere: Part 2. Non-slip surface
• Finite-amplitude thermal convection in a spherical shell

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