Thermally driven hydromagnetic convection in a rapidly rotating sphere

DOI10.1098/rspa.1979.0161zbMath0434.76037OpenAlexW1982485360MaRDI QIDQ3873796

David R. Fearn

Publication date: 1979

Published in: Proceedings of the Royal Society of London. A. Mathematical and Physical Sciences (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1098/rspa.1979.0161

zbMATH Keywords

heat sourceslinear analysismagnetic instabilitygeostrophicself-gravitating fluid sphereBuoyancy-induced convectionRossby instability

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25) Forced convection (76R05) Stability and instability of geophysical and astrophysical flows (76E20) Geo-electricity and geomagnetism (86A25)

Related Items (11)

On the control of rapidly rotating convection by an axially varying magnetic field ⋮ Onset of plane layer magnetoconvection at low Ekman number ⋮ Hydromagnetic waves in a differentially rotating annulus. II. Resistive instabilities ⋮ Non-linear marginal convection in a rotating magnetic system ⋮ Convection-driven hydromagnetic waves in planetary fluid cores. ⋮ Convection in a rotating magnetic system and Taylor's constraint ⋮ Boundary conditions for a rapidly rotating hydromagnetic system in a cylindrical container ⋮ Local analysis of thermal and magnetic instabilities in a rapidly rotating fluid ⋮ Hydromagnetic waves in a differentially rotating Annulus I. A test of local stability analysis ⋮ Thermal and magnetic instabilities in a rapidly rotating fluid sphere ⋮ Quasi-free-decay magnetic modes in planetary cores

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