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• W2171108575 abstract "Abstract An inviscid, electrically conducting fluid is contained between two rigid horizontal planes and bounded laterally by two vertical walls. The fluid is permeated by a strong uniform horizontal magnetic field aligned with the side wall boundaries and the entire system rotates rapidly about a vertical axis. The ratio of the magnitudes of the Lorentz and Coriolis forces is characterized by the Elsasser number, A, and the ratio of the thermal and magnetic diffusivities, q. By heating the fluid from below and cooling from above the system becomes unstable to small perturbations when the adverse density gradient as measured by the Rayleigh number, R, is sufficiently large. With the viscosity ignored the geostrophic velocity, U, which is aligned with the applied magnetic field, is independent of the coordinate parallel to the rotation axis but is an arbitrary function of the horizontal cross-stream coordinate. At the onset of instability the value of U taken ensures that Taylor's condition is met. Specifi..." @default.
• W2171108575 created "2016-06-24" @default.
• W2171108575 creator A5036638743 @default.
• W2171108575 date "1986-01-01" @default.
• W2171108575 modified "2023-09-25" @default.
• W2171108575 title "Non-linear marginal convection in a rotating magnetic system" @default.
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• W2171108575 doi "https://doi.org/10.1080/03091928608245898" @default.
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