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Earth, Planets and Space
Fig. 7 | Earth, Planets and Space

Fig. 7

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. 7

Estimated acceleration waveforms for the blind prediction Step 2 after the time shift. The estimated acceleration waveforms for the blind prediction Step 2 after the time shift (red traces) are compared with the recorded acceleration waveforms (black traces), which were distributed after the blind prediction. 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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