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Earth, Planets and Space
Fig. 11 | Earth, Planets and Space

Fig. 11

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. 11

Comparison of observed and simulated waveforms for the Mw5.5 earthquake. The observed waveform at TVU has a higher amplification than the simulated waveforms. A comparison of results from the initial model (gray) and adjusted model (red) show that a better agreement is obtained when using the adjusted model. Waveform matching was conducted using trial and error for time windows indicated by the red arrows

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