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Nature. 2010 Dec 16;468(7326):952-4. doi: 10.1038/nature09643.

Tidal dissipation and the strength of the Earth's internal magnetic field.

Author information

1
Department of Earth and Planetary Science, University of California, Berkeley, California 94720, USA. bbuffett@berkeley.edu

Abstract

Magnetic fields at the Earth's surface represent only a fraction of the field inside the core. The strength and structure of the internal field are poorly known, yet the details are important for our understanding of the geodynamo. Here I obtain an indirect estimate for the field strength from measurements of tidal dissipation. Tidally driven flow in the Earth's liquid core develops internal shear layers, which distort the internal magnetic field and generate electric currents. Ohmic losses damp the tidal motions and produce detectable signatures in the Earth's nutations. Previously reported evidence of anomalous dissipation in nutations can be explained with a core-averaged field of 2.5 mT, eliminating the need for high fluid viscosity or a stronger magnetic field at the inner-core boundary. Estimates for the internal field constrain the power required for the geodynamo.

PMID:
21164483
DOI:
10.1038/nature09643

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