Geodynamo theory and simulations

Paul H. Roberts and Gary A. Glatzmaier
Rev. Mod. Phys. 72, 1081 – Published 1 October 2000
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Abstract

80 years ago, Joseph Larmor planted the seed that grew into today’s imposing body of knowledge about how the Earth’s magnetic field is created. His simple idea, that the geomagnetic field is the result of dynamo action in the Earth’s electrically conducting, fluid core, encountered many difficulties, but these have by now been largely overcome, while alternative proposals have been found to be untenable. The development of the theory and its current status are reviewed below. The basic electrodynamics are summarized, but the main focus is on dynamical questions. A special study is made of the energy and entropy requirements of the dynamo and in particular of how efficient it is, considered as a heat engine. Particular attention is paid to modeling core magnetohydrodynamics in a way that is tractable but nevertheless incorporates the dynamical effects of core turbulence in an approximate way. This theory has been tested by numerical integrations, some results from which are presented. The success of these simulations seems to be considerable, when measured against the known geomagnetic facts summarized here. Obstacles that still remain to be overcome are discussed, and some other future challenges are described.

    DOI:https://doi.org/10.1103/RevModPhys.72.1081

    ©2000 American Physical Society

    Authors & Affiliations

    Paul H. Roberts

    • Institute of Geophysics and Planetary Physics, University of California, Los Angeles, California 90095

    Gary A. Glatzmaier

    • Department of Earth Sciences, University of California, Santa Cruz, California 95064

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    Issue

    Vol. 72, Iss. 4 — October - December 2000

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