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Morphology of the geomagnetic field and implications for the geodynamo

Abstract

Maps of the radial component of the magnetic field at the surface of Earth's core for 1715–1980 show, on average, a pattern of four lobes, placed symmetrically about the Equator, and zero flux near the poles. Time variations are largely confined to the Atlantic hemisphere (90° E to 90° W). We propose this average field to be the true dynamo-generated field; that equatorial symmetry is a fundamental consequence of the dynamo equations; and that the polar patches are because of the dynamical influence of the inner core. The main lobes are 120° apart and we propose that the flux from a missing third pair of lobes, which should appear symmetrically near the Greenwich meridian, has been re-distributed by near-surface fluid flow to generate secular variation in the Atlantic hemisphere.

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Gubbins, D., Bloxham, J. Morphology of the geomagnetic field and implications for the geodynamo. Nature 325, 509–511 (1987). https://doi.org/10.1038/325509a0

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