HR: 1340h
AN: T23A-1204 [Abstracts]
TI: 3D Radial and Azimuthal Anisotropic Structure in North America
AU: * Yuan, H
AF: Berkeley Seismological Lab, 215 McCone Hall, UC Berkeley, Berkeley, CA 84720, United
States
AU: Marone, F
AF: Paul Scherrer Institut, Paul Scherrer Institut, Villigen, 5232, Switzerland
AU: Liu, K
AF: Department of Geological Sciences and Engineering, University of Missouri-Rolla, Rolla,
MO 65409, United States
AU: Gao, S
AF: Department of Geological Sciences and Engineering, University of Missouri-Rolla, Rolla,
MO 65409, United States
AU: Romanowicz, B
AF: Berkeley Seismological Lab, 215 McCone Hall, UC Berkeley, Berkeley, CA 84720, United
States
AB:
We recently developed a 3D tomographic model of the upper mantle beneath North America that includes both
isotropic S velocity structure as well as radial and azimuthal anisotropy (Marone et al., 2007; Marone and
Romanowicz, 2007). This model was constructed from a joint inversion of fundamental and higher mode surface
waveforms together with constraints on azimuthal anisotropy derived from SKS splitting measurements. This
model showed evidence for the presence of two layers of anisotropy beneath the stable part of the North
American continent: a deeper layer with Vsh>Vsv and with the fast axis direction aligned with the absolute plate
motion direction suggesting lattice preferred orientation of anisotropic minerals in a present day asthenospheric
flow and a shallower lithospheric layer likely showing records of past tectonic events. Under the tectonically active
western US, where the lithosphere is thin, the direction of tomographically inferred anisotropy is stable with depth
and compatible with the absolute plate motion direction.
We here present an updated model, which includes a larger waveform data set (three more years of data
including new data from US Array) and a larger SKS splitting dataset. In addition, we are going one step further in
that we now combine the results from inversion for radial and azimuthal anisotropy, to recover the distribution of
the direction and amplitude of the fast axis in 3D, under the assumptions of hexagonal symmetry. We discuss the
results in the light of possible causes of anisotropy in the cratonic lithosphere.
DE: 7208 Mantle (1212, 1213, 8124)
DE: 7255 Surface waves and free oscillations
DE: 7270 Tomography (6982, 8180)
DE: 8120 Dynamics of lithosphere and mantle: general (1213)
SC: Tectonophysics [T]
MN: 2007 Fall Meeting