Zhang, K. and Gubbins, D. (2000) Scale disparities and magnetohydrodynamics in the Earth’s core. Philosophical Transactions Of The Royal Society Of London Series A - Mathematical Physical and Engineering Sciences, 358 (1768). pp. 899-920. ISSN 1471-2962Full text available as:
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Fluid motions driven by convection in the Earth’s fluid core sustain geomagnetic fields by magnetohydrodynamic dynamo processes. The dynamics of the core is critically influenced by the combined effects of rotation and magnetic fields. This paper attempts to illustrate the scale-related difficulties in modelling a convection-driven geodynamo by studying both linear and nonlinear convection in the presence of imposed toroidal and poloidal fields. We show that there exist three extremely large disparities, as a direct consequence of small viscosity and rapid rotation of the Earth’s fluid core, in the spatial, temporal and amplitude scales of a convection-driven geodynamo. We also show that the structure and strength of convective motions, and, hence, the relevant dynamo action, are extremely sensitive to the intricate dynamical balance between the viscous, Coriolis and Lorentz forces; similarly, the structure and strength of the magnetic field generated by the dynamo process can depend very sensitively on the fluid flow. We suggest, therefore, that the zero Ekman number limit is strongly singular and that a stable convection-driven strong-field geodynamo satisfying Taylor’s constraint may not exist. Instead, the geodynamo may vacillate between a strong field state, as at present, and a weak field state, which is also unstable because it fails to convect sufficient heat.
|Copyright, Publisher and Additional Information:||Copyright © 2000 The Royal Society|
|Keywords:||geodynamo, Taylor constraint, Earth’s core, magnetoconvection|
|Academic Units:||The University of Leeds > Faculty of Environment (Leeds) > School of Earth and Environment (Leeds)|
|Depositing User:||Repository Officer|
|Date Deposited:||23 Mar 2005|
|Last Modified:||08 Feb 2013 17:01|
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