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Automated SKS splitting and upper-mantle anisotropy beneath ... - bris

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<strong>Automated</strong> <strong>SKS</strong> <strong>splitting</strong> 941Figure 9. The top plot shows polarization directions of corrected <strong>SKS</strong> phasesusing the eigenvalue method plotted against backazimuth at WALA. Thepredicted backazimuth is shown by the dashed line. There is a distinct biastowards larger polarization values consistent with anticlockwise misalignment,(mean offset 12 ◦ ). The bottom plot shows polarization directions ofdirect P arrivals measured at the same station, (mean offset 8 ◦ ).Figure 11. Splitting measurements in relation to APM <strong>and</strong> tectonics of theInnuitian orogeny. There is good correlation between <strong>splitting</strong> measurements<strong>and</strong> the trend of faults related to the Proterozoic Innuitian orogen (taken fromOkulitch (1991).Figure 12. Splitting measurements in relation to APM <strong>and</strong> tectonics of theAppalachian orogeny. Fault trends taken from Wheeler et al. (1996).Figure 10. Correlation between <strong>splitting</strong> measurements, tectonic features<strong>and</strong> APM directions for stations in Western Canada. T.T.: Tintina Trench.R.M.T. Rocky Mountain Trench G.S.L.S.Z.: Great Slave Lake Shear Zone.S.T.Z.: Snowbird Tectonic Zone. Orientation of geological features fromHoffman (1989); Wheeler et al. (1991, 1996). Arrows are estimates of currentday APM taken from DeMets et al. (1994), Kreemer et al. (2003) <strong>and</strong> Gripp& Gordon (2002). APM estimates for PGC are those of the subducting Ju<strong>and</strong>e Fuca plate, rather than the North American plate.of the IRIS Data Management Centre. We would also like to thankthe International Seismological Centre for providing Bulletin data<strong>and</strong> the continued use of their computing facilities, <strong>and</strong> the staff ofthe Czech Academy of Sciences for assistance with <strong>splitting</strong> codesin the early stages of this project.The IRIS DMS is funded through the National Science Foundation<strong>and</strong> specifically the GEO Directorate through the Instrumentation<strong>and</strong> Facilities Program of the National Science Foundationunder Cooperative Agreement EAR–0004370.Funding for this project was provided by NERC grant NER/A/S/2001/00524.C○ 2006 The Authors, GJI, 165, 931–942Journal compilation C○ 2006 RAS

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