Hydromagnetic edge waves in a rotating stratified fluid

Author:

Andrews D. G.,Hide R.

Abstract

The properties of edge waves confined by the interaction of buoyancy and Coriolis forces to the vicinity of a rigid plane boundary in a rotating, stratified, electrically conducting fluid pervaded by a magnetic field are established in some simple cases. The background shear is taken to be zero, the basic Alfvén velocity V and Brunt–Väisälä frequency N are assumed uniform, and all dissipative effects are taken to be vanishingly small. It is shown that waves trapped against the bounding wall can occur only if V is parallel to the wall. When the basic rotation vector Ω is also parallel to the wall, the hydromagnetic edge waves have a higher frequency and smaller spatial extent perpendicular to the wall than their non-hydromagnetic counterparts, but more complex behaviour is found when Ω possesses a component normal to the wall. There are conditions under which edge waves may exist even when the basic density stratification is top-heavy (i.e. when N2 < 0).

Publisher

Cambridge University Press (CUP)

Subject

Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics

Reference11 articles.

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2. Skiles, D. D. 1972 On the transmission of energy in an incompressible magnetohydrodynamic wave into a conducting solid.Phys. Earth Planet. Interiors,5,99–109.

3. Hide, R. & Stewartson, K. 1972 Hydromagnetic oscillations of the Earth's core.Rev. Geophys. Space Phys. 10,579–598.

4. Rhines, P. B. 1970 Edge-, bottom-, and Rossby waves in a rotating stratified fluid.Geophys. Fluid Dyn. 1,273–302.

5. Hide, R. 1969b The viscous boundary layer at the rigid bounding surface of an electrically-conducting rotating fluid in the presence of a magnetic field.J. Atmos. Sci. 26,847–853.

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