The existence of a thin low-viscosity layer beneath the lithosphere

Details The existence of a thin low-viscosity layer beneath the lithosphere The existence of a thin low-viscosity layer beneath the lithosphere

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986e%26psl..78..420c&link_type=abstract

Earth and Planetary Science Letters (ISSN 0012-821X), vol. 78, no. 4, July 1986, p. 420-426.

Physics

55

Crustal Fractures, Geotemperature, Lithosphere, Ocean Bottom, Plates (Tectonics), Satellite Observation, Bathymeters, Convective Heat Transfer, Geoids, Seasat Satellites, Temperature Gradients, Two Dimensional Models, Viscosity

Scientific paper

The horizontal temperature gradient at the base of the lithosphere at an oceanic fracture zone, where plate of different ages is juxtaposed, is expected to drive a local circulation, the characteristics of which can be constrained by the amplitude, wavelength and age-dependence of the geoid. Two-dimensional numerical models of convection in a fluid layer overlain by a solid conducting lid have been used to generate theoretical geoid profiles at right angles to the fracture zone. Only a thin, low-viscosity layer provides a reasonable fit to the data. The best model so far obtained has a fluid layer 150 km thick with viscosity 1.5 times 10 to the 19th Pa s under a 75 km lid. Such a layer, which is incapable of transmitting strong horizontal shear stresses, could provide the decoupling mechanism between plate and deep mantle flow required to balance the forces on the plates.

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