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Earth, Planets and Space
Fig. 3 | Earth, Planets and Space

Fig. 3

From: Estimation of shallow S-wave velocity structure using microtremor array exploration at temporary strong motion observation stations for aftershocks of the 2016 Kumamoto earthquake

Fig. 3

a Observed phase velocity at MK01 (circles) and the calculated phase velocity curve for the best-fit model (gray line). The curves that differ from the best-fit curve by a maximum of 1% (acceptable curves) are shown as thin solid lines. b V S profiles for the best-fit phase velocity curve (gray) and acceptable curves (thin solid line). c Amplification for the best-fit model (gray) and acceptable models (thin solid line)

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