Seismic velocity structure and depth-dependence of anisotropy in the Red Sea and Arabian shield from surface wave analysis

Publication Type  Journal Article
Year of Publication  2008
Authors  Hansen, S. E.; Gaherty, J. B.; Schwartz, S. Y.; Rodgers, A. J.; Al-Amri, A. M. S.
Journal Title  Journal of Geophysical Research-Solid Earth
Volume  113
Issue  B10
Pages  -
Journal Date  Oct 14
ISBN Number  0148-0227
Accession Number  ISI:000260180000002
Key Words  upper-mantle structure; continental upper-mantle; azimuthal anisotropy; lithospheric structure; saudi-arabia; receiver functions; uppermost mantle; kaapvaal craton; plate-motion; simple-shear
Abstract  

We investigate the lithospheric and upper mantle shear wave velocity structure and the depth-dependence of anisotropy along the Red Sea and beneath the Arabian Peninsula using receiver function constraints and phase velocities of surface waves traversing two transects of stations from the Saudi Arabian National Digital Seismic Network. Frequency-dependent phase delays of fundamental-mode Love and Rayleigh waves, measured using a cross-correlation procedure, require very slow shear velocities and the presence of anisotropy to depths of at least 180 km in the upper mantle. Linearized inversion of these data produce path-averaged 1D radially anisotropic models with similar to 4% anisotropy in the lithosphere and across the lithosphere-asthenosphere boundary (LAB). Models with reasonable crustal velocities in which the mantle lithosphere is isotropic cannot satisfy the data. The lithosphere, which ranges in thickness from about 70 km near the Red Sea coast to about 90 km beneath the Arabian Shield, is underlain by a pronounced low-velocity zone with shear velocities as low as 4.1 km/s. Forward models of azimuthal anisotropy, which are constructed from previously determined shear wave splitting estimates, can reconcile surface and body wave observations of anisotropy. The low shear velocities extend to greater depth than those observed in other continental rift and oceanic ridge environments. The depth extent of these low velocities combined with the sharp velocity contrast across the LAB may indicate the influence of the Afar hot spot and the presence of partial melt beneath Arabia. The anisotropic signature primarily reflects a combination of plate- and density-driven flow associated with rifting processes in the Red Sea.

Notes  

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URL  <Go to ISI>://000260180000002
DOI  Doi 10.1029/2007jb005335