Convection-driven hydromagnetic waves in planetary fluid cores.

DOI10.1016/S0895-7177(02)00133-4zbMath1129.85304OpenAlexW2088444550WikidataQ56326404 ScholiaQ56326404MaRDI QIDQ1410113

D. Gubbins, Keke Zhang

Publication date: 14 October 2003

Published in: Mathematical and Computer Modelling (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/s0895-7177(02)00133-4

zbMATH Keywords

Magnetohydrodynamic wavesGeodynamoMagnetoconvectionTangent cylinder

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Cites Work

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• Kinematic dynamo action in a sphere. I. Effects of differential rotation and meridional circulation on solutions with axial dipole symmetry
• Hydromagnetic waves in a differentially rotating sphere
• Thermal and magnetic instabilities in a rapidly rotating fluid sphere
• Thermally driven hydromagnetic convection in a rapidly rotating sphere
• Hydromagnetic convective instability of a rotating, self-gravitating fluid sphere containing a uniform distribution of heat sources
• Thermal and magnetically driven convection in a rapidly rotating fluid layer
• Scale disparities and magnetohydrodynamics in the Earth's core
• Spherical shell rotating convection in the presence of a toroidal magnetic field
• On hydromagnetic instabilities driven by the Hartmann boundary layer in a rapidly rotating sphere
• Hydromagnetic planetary waves

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