Hydromagnetic convective instability of a rotating, self-gravitating fluid sphere containing a uniform distribution of heat sources

DOI10.1098/rspa.1977.0026zbMath0392.76040OpenAlexW2146015213MaRDI QIDQ4174410

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Publication date: 1977

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.1977.0026

zbMATH Keywords

Heat SourcesBoussinesq ApproximationConvective InstabilityRotatingChandrasekhar NumberCritical Rayleigh NumberHydromagneticPlanetary Magnetic FieldSelf-GravitatingTaylor Number

Mathematics Subject Classification ID

Magnetohydrodynamics and electrohydrodynamics (76W05) Stability and instability of magnetohydrodynamic and electrohydrodynamic flows (76E25)

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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 ⋮ On the propagation of hydromagnetic- inertial-gravity waves in magnetic-velocity shear ⋮ Hydromagnetic waves in the Earth's fluid core ⋮ Convection-driven hydromagnetic waves in planetary fluid cores. ⋮ Future of geodynamo theory ⋮ Convection in a rotating magnetic system and Taylor's constraint ⋮ On steady kinematic helical dynamos ⋮ Nonlinear convection in an imposed horizontal magnetic field ⋮ Thermal and magnetic instabilities in a rapidly rotating fluid sphere ⋮ On the propagation and stability of wave motions in rapidly rotating spherical shells: I. The non-magnetic case

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