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Fig. 6 | Earth, Planets and Space

Fig. 6

From: XYtracker: a new approach to estimate fault rupture extent in real time for large earthquakes

Fig. 6

Distribution of the seismic intensity and its error at 180 s for the 2011 Tohoku earthquake. The observation and the estimations of the PS, LS, and RS models are shown from the left. Black stars and thick lines show the epicenters and the source models, respectively. a Observed intensity. b–d Estimated intensity for the 3 source models. e–g Difference between the estimated and observed intensities for the 3 source models. h–j Scatter plot of the observed and estimated intensities for the 3 source models. The red color indicates over-predicted, and the blue color shows under-predicted. The percentage of the stations with an error > 1 is written in the panel

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