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  • 1
    Publication Date: 2012-05-01
    Description: INTRODUCTION As early as the 1920s, Gutenberg (1926) equated the low-viscosity asthenosphere with a seismic low-velocity zone. Regions of high and low velocity in the mantle are today usually determined with tomographic methods. These methods are, however, not very sensitive to sharp boundaries. Converted waves have been used for many years to study boundaries in the mantle. A velocity reduction with depth (possibly the lithosphere-asthenosphere boundary, LAB) was found with P-to-S converted waves (P-receiver functions) beneath North America at ∼100 km depth with a sharpness of about 10 km (Rychert and Shearer 2009). A comparison of the LAB depth from S-receiver functions (see, e.g., Yuan et al. 2006 and Kumar et al. 2006 for a description of the method and data examples) with that from surface-wave tomography found good agreement in the western United States (Li et al. 2007) and along the East Coast (Rychert et al. 2007). Our results from the California coast are also consistent with the P-to-S and S-to-P images earlier analyzed by Kumar and Kawakatsu (2011), along a profile spanning ocean to continent. A discrepancy exists in the central part of the craton, where the sharp velocity decrease at about 100 km in P-receiver functions (PRF) was confirmed with S-receiver functions (SRF) in contrast to the smooth velocity decrease around 200 km depth known from surface-wave data (Yuan and Romanowicz 2010; Abt et al. 2010; Yuan et al. 2011). The petrophysical nature of the LAB is still very much a subject of discussion (e.g., Eaton et al. 2009; Fischer et al. 2010). We think our results from USArray data significantly contribute to this discussion. The earlier results were obtained with relatively few, sparsely distributed seismic stations (Abt et al. 2010). We apply...
    Print ISSN: 0895-0695
    Electronic ISSN: 1938-2057
    Topics: Geosciences
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  • 2
    Publication Date: 2011-06-01
    Description: The collision of the Indian and Asian plates since about 55 Ma has created the largest plateau with the thickest crust on Earth. There is, however, no general agreement on the modes of the crustal thickening. The crustal thickness of the Tibetan plateau still remains poorly determined. It is generally accepted that the Tibetan crust has roughly double normal thickness and that it thins somewhat toward the north, but individual observations of Moho depth vary spatially and for different techniques at the same place by greater than 20 km. In this work we compare P and S receiver functions at station LSA, located in the southern Lhasa terrane, to determine the crustal thickness beneath the station. A doublet Moho structure with two significant interfaces at about 60 and 80 km depth in the lower crust is seen clearly in the P receiver functions. The deeper phase (Moho) is, however, absent in the S receiver function data. Here we model the observed P and S receiver functions by a strong Moho topography that dips to the east at an angle of 30{degrees}. This result may indicate that the Moho structure beneath Tibet can be very complicated and has strong lateral variations and suggests that a detailed map of Moho depth is only possible with 2D dense seismic experiments. The Moho dips locally perpendicular to the direction of the Indian plate motion, suggesting that the lower crustal deformation is decoupled from the underlying Indian mantle lithosphere. The extremely strong Moho variation beneath and east of station LSA may also imply a crust-mantle interaction, specifically delamination or foundering of lower crust down to the upper mantle.
    Print ISSN: 0037-1106
    Electronic ISSN: 1943-3573
    Topics: Geosciences , Physics
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