Toroidal flux oscillation as possible cause of geomagnetic excursions and reversals

Busse, F.H. and Simitev, R.D. (2008). Toroidal flux oscillation as possible cause of geomagnetic excursions and reversals. Physics of the Earth and Planetary Interiors, 168 (3-4), pp. 237-243.

Abstract

It is proposed that convection driven dynamos operating in planetary cores could be oscillatory even when the oscillations are not directly noticeable from the outside. Examples of dynamo simulations are pointed out that exhibit oscillations in the structure of the azimuthally averaged toroidal magnetic flux while the mean poloidal field shows only variations in its amplitude. In the case of the geomagnetic field, global excursions may be associated with these oscillations. Long period dynamo simulations indicate that the oscillations may cause reversals once in a while. No special attempt has been made to use most realistic parameter values. Nevertheless some similarities between the simulations and the paleomagnetic record can be pointed out. Crown

Publication DOI: https://doi.org/10.1016/j.pepi.2008.06.007
Divisions: Engineering & Applied Sciences > Mathematics
Engineering & Applied Sciences > Systems analytics research institute (SARI)
Additional Information: © 2009, Elsevier. Licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International http://creativecommons.org/licenses/by-nc-nd/4.0/
Uncontrolled Keywords: geodynamo,excursions,reversal,dynamo oscillations
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Related URLs: http://www.scop ... tnerID=8YFLogxK (Scopus URL)
Published Date: 2008-07
Authors: Busse, F.H.
Simitev, R.D.

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