Skip to main content
Fig. 7 | Earth, Planets and Space

Fig. 7

From: A look at the blind Kumamoto experiment: combining active and passive seismic observations to avoid Rayleigh-wave mode misidentification

Fig. 7

High-res MASW; Forward (a) and reverse (b) direction high-resolution MASW images computed with the deblurring method (Mikesell et al. 2017). In addition, the two near-offset traces (1.5 and 3.0 m) were removed from the shot records (Fig. 3) prior to applying the MASW. A velocity-based window is also applied to time series from 50 to 600 m/s to remove energy outside this velocity range prior to MASW. Solid curves are predicted modes for “preferred model” (Table 3)

Back to article page