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Fig. 6 | Earth, Planets and Space

Fig. 6

From: Kinematic source models for long-period ground motion simulations of megathrust earthquakes: validation against ground motion data for the 2003 Tokachi-oki earthquake

Fig. 6

Distributions of source parameters. a Rake angle, b rupture time, and c slip of Models 0, C, H1H3, and S1S3. For Model 0, the rake angles and rupture time of the time window in which the peak slip velocity occurs are plotted. The rupture time distribution of Models C and H1 differs from that of Model S3 because they consider multiple hypocenters

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