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P 9.4267BLDU45P 20.1213CASY39P 2.6205MAW57P 13.6181SBA34P 3.0181SNAA64P 13.8156PMSA63P 9.3128LCO87P 40.563PPTF41P 50.955RAR32P 52.139XMAS53P 31.330AFI32P 22.029KIP70P 17.220JOHN62P 28.71TARA44−10 0 10 20 30 40 50t(s)SH 100.339XMAS53P 22.1354WAKE62P 35.0339HNR35P 9.9339ERM89P 11.7333MAJO85P 18.7330GUMO61P 34.1320PMG40P 29.0311COEN38P 41.1309CTAO31P 27.3298MTN46P 11.3291KSM70P 8.2283PSI79P 18.5283WRKA39P 13.4280MBWA48−10 0 10 20 30 40 50t(s)SH 144.3354WAKE62SH 40.2311COEN38SH 64.8309CTAO31SH 81.8298MTN46SH 42.2291KSM70SH 57.2283PSI79SH 113.7283WRKA39SH 132.8267BLDU45SH 42.3213CASY39SH 184.6181SBA34SH 54.6181SNAA64SH 95.0156PMSA63SH 57.6128LCO87SH 106.863PPTF41−10 0 10 20 30 40 50t(s)F1: Strike= 345 degF2: Strike= 87 degkmkmDepth km01020-10 0 104101010-20 0 20101010101001020Depth km0 100 200 300▲ ▲ Figure 3. Results of the two-segment finite fault inversion. The upper panel shows the displacement waveform fits in black for thedata and red for the synthetic. Station names are displayed to the left of the traces along with the azimuths and epicentral distancesin degrees. Peak amplitude (in microns) for data is indicated above the end of each trace. The lower panel shows the cumulative slipdistribution (slip vectors with amplitude of slip also represented by color shading) and time contours of the rupture propagation asdetermined by the inversion. The rupture times are given relative to the origin time, and the red star indicates the epicenter. The strikeof each segment is shown on the top.cm804 Seismological Research Letters Volume 82, Number 6 November/December 2011

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