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Earth, Planets and Space
Fig. 8 | Earth, Planets and Space

Fig. 8

From: Use of Fourier phase characteristics and effective stress analyses for post-earthquake ground motion estimation: application to ESG6 blind prediction steps 2&3 dataset and JMA accelerometric data

Fig. 8

Estimated velocity waveforms for the blind prediction Step 2 after the time shift. The estimated velocity waveforms for the blind prediction Step 2 after the time shift (red traces) are compared with the velocity waveforms calculated from the records (black traces). The estimated waveforms were shifted so that the arrival time of the S-wave be consistent between the estimated and recorded waveforms

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