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On hydromagnetic instabilities driven by the Hartmann boundary layer in a rapidly rotating sphere

Published online by Cambridge University Press:  26 April 2006

Keke Zhang
Affiliation:
Department of Mathematics, University of Exeter, UK
F. H. Busse
Affiliation:
Institute of Physics, University of Bayreuth, Germany

Abstract

The instability of an electrically conducting fluid of magnetic diffusivity λ and viscosity v in a rapidly rotating spherical container of magnetic diffusivity $\hat{\lambda}$ in the presence of a toroidal magnetic field is investigated. Attention is focused on the case of a toroidal magnetic field induced by a uniform current density parallel to the axis of rotation, which was first studied by Malkus (1967). We show that the internal ohmic dissipation does not affect the stability of the hydromagnetic solutions obtained by Malkus (1967) in the limit of small λ. It is solely the effect of the magnetic Hartmann boundary layer that causes instabilities of the otherwise stable solutions. When the container is a perfect conductor, $\hat{\lambda}$ = 0, the hydromagnetic instabilities grow at a rate proportional to the magnetic Ekman number of the fluid Eλ; when the container is a nearly perfect insulator, $\lambda/\hat{\lambda}\ll 1$, the hydromagnetic instabilities grow at a rate proportional to E1/2λ; when the container is a nearly perfect conductor, λ 1, the growth rates are proportional to λ, where λ is the magnetic Ekman number based on the diffusivity λ of the container. The main characteristics of the instabilities are not affected by varying magnetic properties of the container. In light of the destabilizing role played by the Hartmann boundary layer, we also examine the corresponding magnetoconvection in a rapidly rotating fluid sphere with the perfectly conducting container and stress-free velocity boundary conditions. Analytical magnetoconvection solutions in closed form are obtained and implications are discussed.

Type
Research Article
Copyright
© 1995 Cambridge University Press

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References

Acheson, D. J. 1972 On the hydromagnetic stability of a rotating fluid annulus. J. Fluid Mech. 52, 529541.Google Scholar
Acheson, D. J. 1978 Magnetohydrodynamic waves and stabilities in rotating fluids. In Rotating Fluids in Geophysics (ed. P. H. Roberts & A. M. Soward), pp. 515549. Academic.
Busse, F. H. 1970 Thermal instabilities in rapidly rotating systems. J. Fluid Mech. 44, 441460.Google Scholar
Busse, F. H. 1982 Thermal convection in rotating systems. Proc. 9th US Nat. Congress of Appl. Mech., pp. 299305. ASME
Chandrasekhar, S. 1961 Hydrodynamic and Hydromagnetic Stability. Clarendon Press. ELTAYEB, I. A. 1992 The propagation and stability of linear wave motions in rapidly rotating spherical shells: weak magnetic fields. Geophys. Astrophys. Fluid Dyn. 67, 211240.Google Scholar
Eltayeb, I. A. & Kumar, S. 1977 Hydromagnetic convective instability of a rotating, self-gravitating fluid sphere containing a uniform distribution of heat sources. Proc. R. Soc. Land. A 353, 145162.Google Scholar
Fearn, D. R. 1979a Thermally driven hydrodynamic convection in a rapidly rotating sphere. Proc. R. Soc. Land. A 326, 227242.Google Scholar
Fearn, D. R. 1979 6 Thermal and magnetic instabilities in a a rapidly rotating sphere. Geophys. Astrophys. Fluid Dyn. 14, 103126.Google Scholar
Fearn, D. R. 1983 Hydromagnetic waves in a differentially rotating annulus I. A test of local stability analysis. Geophys. Astrophys. Fluid Dyn. 27, 137162.Google Scholar
Fearn, D. R. 1988 Hydromagnetic waves in a differentially rotating annulus IV. Insulating boundaries. Geophys. Astrophys. Fluid Dyn. 44, 5575.Google Scholar
Fearn, D. R. 1993 Magnetic instabilities in rapidly rotating systems. In Theory of Solar and Planetary Dynamos (ed. M. R. E. Proctor, P. C. Matthews & A. M. Rucklidge), pp. 5968. Cambridge University Press.
Fearn, D. R. & Proctor, M. R. E. 1983 Hydromagnetic waves in a differentially rotating sphere. J. Fluid Mech. 128, 120.Google Scholar
Fearn, D. R. & Weiglhofer, W. S. 1991 Magnetic instabilities in rapidly rotating spherical geometries:!. From cylinders to spheres. Geophys. Astrophys. Fluid Dyn. 56, 159181.Google Scholar
Greenspan, H. P. 1969 The Theory of Rotating Fluids. Cambridge University Press.
Hide, R. 1966 Free hydromagnetic oscillations of the Earth's core and the theory of the geomagnetic secular variation. Phil. Trans R. Soc. Land. A 259, 615647.Google Scholar
Hide, R. & Stewartson, K. 1972 Hydrodynamics oscillations of the Earth's core. Rev. Geophys. Space Phys. 10, 579598.Google Scholar
Jacobs, J. A. 1975 The Earth's Core. Academic Press.
Kerswell, R. R. 1994 Tidal excitation of hydromagnetic waves and their damping in the Earth. J. Fluid Mech. 274, 219241.Google Scholar
Lyttleton, R. A. 1953 The Stability of Rotating Liquid Masses. Cambridge University Press.
Malkus, W. V. R. 1967 Hydromagnetic planetary waves. J. Fluid Mech. 28, 793802Google Scholar
Malkus, W. V. R. 1968 Equatorial planetary waves. Tellus 20, 545547Google Scholar
Proctor, M. R. E. 1994 Magnetoconvection in a rapidly rotating sphere. In Stellar and Planetary Dynamos (ed. M. R. E. Proctor & A. D. Gilbert). Cambridge University Press.
Roberts, P. H. & Loper, D. E. 1979 On the diffusive instability of some simple steady magneto- hydrodynamic flows. J. Fluid Mech. 90, 641668.Google Scholar
Soward, A. M. 1979 Thermal and magnetically driven convection in a rapidly rotating fluid layer. J. Fluid Mech. 90, 669684.Google Scholar
Zhang, K. 1993 On equatorially trapped boundary inertial waves. J. Fluid Mech. 248, 203217.Google Scholar
Zhang, K. 1994 On coupling between the Poincaré equation and the heat equation. J. Fluid Mech. 268, 211229.Google Scholar
Zhang, K. 1995a On coupling between the Poincaré equation and the heat equation :non-slip boundary condition. J. Fluid Mech. 284, 239256.Google Scholar
Zhang, K. 1995c Spherical shell rotating convection in the presence of a toroidal magnetic field. Proc R. Soc. Land. A 448, 123.Google Scholar
Zhang, K. & Fearn, D. 1993 How strong is the invisible component of the magnetic field in the Earth's core? Geophys. Res. Lett. 20, 20832088.Google Scholar
Zhang, K. & Fearn, D. R. 1994 Hydromagnetic waves in a rotating spherical shell generated by toroidal magnetic fields. Geophys. Astrophys. Fluid Dyn. 77, 133157.Google Scholar