Linear Magnetoconvection in Rotating Fluid Spheres Permeated by a Uniform Axial Magnetic Field
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Publication:3080114
DOI10.1080/03091920290024234zbMath1206.86037OpenAlexW2079736677MaRDI QIDQ3080114
Publication date: 5 March 2011
Published in: Geophysical & Astrophysical Fluid Dynamics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1080/03091920290024234
General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Convection in hydrodynamic stability (76E06) Geo-electricity and geomagnetism (86A25)
Related Items (3)
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field ⋮ A detailed analysis of a dynamo mechanism in a rapidly rotating spherical shell ⋮ The cross-over to magnetostrophic convection in planetary dynamo systems
Cites Work
- Thermal and magnetic instabilities in a rapidly rotating fluid sphere
- Spiralling columnar convection in rapidly rotating spherical fluid shells
- Magnetohydrodynamics in Rapidly Rotating spherical Systems
- Spherical shell rotating convection in the presence of a toroidal magnetic field
- Imposing a magnetic field across a nonaxisymmetric shear layer in a rotating spherical shell
- Thermal instability in a horizontal fluid layer: effect of boundary conditions and non-linear temperature profile
- Influence of an Axial Magnetic Field on the Steady Linear Ekman Boundary Layer
- On the thermal instability of a rotating-fluid sphere containing heat sources
- Thermal instabilities in rapidly rotating systems
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