Magnetoconvection in a rapidly rotating sphere: the weak–field case

DOI10.1098/rspa.2002.1048zbMath1116.76355OpenAlexW2135082398MaRDI QIDQ4470787

Chris A. Jones, Ali I. Mussa, Steven J. Worland

Publication date: 15 June 2004

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

Full work available at URL: https://doi.org/10.1098/rspa.2002.1048

zbMATH Keywords

Ekman numberglobal asymptotic theoryElsasser numberlinear stability of magnetoconvectionWentzel-Kramers-Brillouin solution

Mathematics Subject Classification ID

General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Convection in hydrodynamic stability (76E06) Stability and instability of geophysical and astrophysical flows (76E20) Geo-electricity and geomagnetism (86A25)

Related Items (5)

On the control of rapidly rotating convection by an axially varying magnetic field ⋮ Helicity generation and subcritical behaviour in rapidly rotating dynamos ⋮ Confinement of rotating convection by a laterally varying magnetic field ⋮ A multiscale dynamo model driven by quasi-geostrophic convection ⋮ Azimuthal winds, convection and dynamo action in the polar regions of planetary cores

This page was built for publication: Magnetoconvection in a rapidly rotating sphere: the weak–field case