Convection driven magnetohydrodynamic dynamos in rotating spherical shells

DOI10.1080/03091928908243466zbMath0683.76097OpenAlexW1978097262MaRDI QIDQ4733623

Keke Zhang, Friedrich H. Busse

Publication date: 1989

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

Full work available at URL: https://doi.org/10.1080/03091928908243466

zbMATH Keywords

Galerkin methodLorentz forcerotating spherical fluid shellsFinite amplitude solutionsmagnetohydrodynamic dynamos driven by convectionnon- magnetic solutions

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Forced convection (76R05) Basic methods in fluid mechanics (76M99)

Related Items (6)

Estimates for the effective electrical conductivity of the core in the interior of Jupiter and Saturn ⋮ On the internal structure and magnetic fields of venus ⋮ Quasi-geostrophic motions in a rotating layer of an electrically conducting fluid ⋮ Computing with Functions in the Ball ⋮ Convective flows in rapidly rotating spheres and their dynamo action ⋮ An efficient numerical scheme for a 3D spherical dynamo equation

Cites Work

• On the onset of convection in rotating spherical shells
• Finite amplitude convection and magnetic field generation in a rotating spherical shell
• Thermal instabilities in rapidly rotating systems

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