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Fig. 9 | Earth, Planets and Space

Fig. 9

From: Estimation of 1-D velocity models beneath strong-motion observation sites in the Kathmandu Valley using strong-motion records from moderate-sized earthquakes

Fig. 9

Simulation of the Mw5.1 earthquake using the adjusted velocity model. The observed amplification at TVU is larger than the simulated waveform. The gray waveform is the result from the Propagator Matrix method using the initial velocity model. Waveform matching was conducted using trial and error for time windows indicated by the red arrows

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