Radial Seismic Anisotropy As a Constraint for Upper Mantle Rheology ⁎ Thorsten W
Available online at www.sciencedirect.com Earth and Planetary Science Letters 267 (2008) 213–227 www.elsevier.com/locate/epsl Radial seismic anisotropy as a constraint for upper mantle rheology ⁎ Thorsten W. Becker a, , Bogdan Kustowski b, Göran Ekström c a Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA b Department of Earth and Planetary Sciences, Harvard University, Cambridge MA, USA c Department of Earth and Environmental Sciences, Lamont-Doherty Earth Observatory, Palisades, NY, USA Received 26 July 2007; received in revised form 9 November 2007; accepted 22 November 2007 Available online 8 December 2007 Editor: R.D. van der Hilst Abstract Seismic shear waves that are polarized horizontally (SH) generally travel faster in the upper mantle than those that are polarized vertically (SV), and deformation of rocks under dislocation creep has been invoked to explain such radial anisotropy. Convective flow of the upper mantle may thus be constrained by modeling the textures that progressively form by lattice-preferred orientation (LPO) of intrinsically anisotropic grains. While azimuthal anisotropy has been studied in detail, the radial kind has previously only been considered in semi-quantitative models. Here, we show that radial anisotropy averages as well as radial and azimuthal anomaly-patterns can be explained to a large extent by mantle flow, if lateral viscosity variations are taken into account. We construct a geodynamic reference model which includes LPO formation based on mineral physics and flow computed using laboratory-derived olivine rheology. Previously identified anomalous vSV regions beneath the East Pacific Rise and relatively fast vSH regions within the Pacific basin at ~150 km depth can be linked to mantle upwellings and shearing in the asthenosphere, respectively.
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