Numerical simulations of thermal-chemical instabilities at the core–mantle boundary (original) (raw)
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- Published: 21 July 1988
Nature volume 334, pages 237–240 (1988) Cite this article
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Abstract
Dynamical effects at the core–mantle boundary have so far been modelled mainly with thermal convection1,2, yet accumulating evidence3,4 supports the idea of a combined thermal and chemical boundary layer as the likely explanation of the D″ zone. Here we present numerical simulations of thermal-chemical instabilities in the D″ layer which show that strong lateral heterogeneities in the composition and density fields can be initiated and maintained dynamically if there is continuous replenishment of material from subduced slabs coming from the upper mantle. These chemical instabilities have a tendency to migrate laterally and may help to support core–mantle boundary topography with short and long wavelengths. The thermal-chemical flows produce a relatively stagnant D″ layer with strong lateral and temporal variations in basal heat flux, which gives rise to thermal core–mantle interactions5, influencing the geodynamo.
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Authors and Affiliations
- Institut für Geophysik und Meteorologie, Universität zu Köln, D-5000, Köln, 41, FRG
Ulrich Hansen - Minnesota Supercomputer Institute and Department of Geology and Geophysics, University of Minnesota, Minneapolis, Minnesota, 55455, USA
David A. Yuen
Authors
- Ulrich Hansen
- David A. Yuen
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Hansen, U., Yuen, D. Numerical simulations of thermal-chemical instabilities at the core–mantle boundary.Nature 334, 237–240 (1988). https://doi.org/10.1038/334237a0
- Received: 05 January 1988
- Accepted: 01 June 1988
- Issue date: 21 July 1988
- DOI: https://doi.org/10.1038/334237a0
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