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Fig. 3 | Earth, Planets and Space

Fig. 3

From: Joint inversion of teleseismic and InSAR datasets for the rupture process of the 2010 Yushu, China, earthquake

Fig. 3

(a) Variations in teleseismic misfit as a function of rupture front velocity (V i ). (b) Snapshots of the slip distribution of the best-fitting model. Solid and dashed white circles indicate rupture propagation at speeds of 4.7 and 3.5 km/s. (c) (upper) Comparison of the observed and synthetic waveforms from the joint inversion. The number above the station code denotes the peak-to-peak value of the observed record in micrometers, whereas the number below the station code is the station azimuth measured from the source. (lower) Comparison of the InSAR LOS observations and the calculations from the joint inversion in quadtree blocks. (d) Variations in misfit as a function of rupture front velocity (V i ) in models using other subfault sizes (left) and rise times (right). (e) Resultant slip distribution obtained by the finite source inversion using the teleseismic waveform data and InSAR data. The black star and arrows indicate the hypocenter and the subfault slips on the hanging wall, respectively.

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