TRACKING GEOMAGNETIC IMPULSES AT THE CORE-MANTLE BOUNDARY

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dc.contributor.author Dormy E.
dc.contributor.author Mandea M.
dc.date.accessioned 2023-12-30T07:21:41Z
dc.date.available 2023-12-30T07:21:41Z
dc.date.issued 2005
dc.identifier https://www.elibrary.ru/item.asp?id=31338052
dc.identifier.citation Earth and Planetary Science Letters, 2005, 237, 1-2, 300-309
dc.identifier.issn 0012-821X
dc.identifier.uri https://repository.geologyscience.ru/handle/123456789/42399
dc.description.abstract The main magnetic field of the Earth is generated and maintained by convective motions in the fluid outer core. Temporal field variations occur on an impressive variety of scales, ranging from months to millions of years. Among these, the most intriguing features are geomagnetic "impulses" or "jerks" [V. Courtillot, J. Ducruix and J.L. Le Mouël, Sur une accélération récente de la variation séculaire du champ magnétique terrestre, Acad. Sci. Paris C.R., D287, (1978) 1095-1098., J.L. Le Mouël, J. Ducruix and C. Ha Duyen, Geophys. Res. Lett., 5, (1983) 369. [1,2]]. Here, we investigate these very rapid events at the surface of the Earth's core using a global model, designed for use at this depth. We identify two regions of very active variations, where wave-like structures propagate. The geometrical characteristics of these wave-like motions provide new constraints on the intricate dynamics of the core. © 2005 Elsevier B.V. All rights reserved.
dc.subject GEODYNAMO
dc.subject GEOMAGNETISM
dc.subject SECULAR VARIATION
dc.title TRACKING GEOMAGNETIC IMPULSES AT THE CORE-MANTLE BOUNDARY
dc.type Статья
dc.identifier.doi 10.1016/j.epsl.2005.06.003


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