Electronic Supplement to

Dynamic Rupture Models for the Southern San Andreas Fault

by Geoffrey P. Ely, Steven M. Day, and Jean-Bernard Minster

Movie 1: Rupture Dynamics

Animation of normal traction, shear traction, slip, peak slip rate, and slip rate on the fault surface for model 4T. Vertical lines mark changes in strike between planar segments. The star marks the nucleation point at 5 km depth. On each plot, slip path length is contoured at the initiation of rupture and at the slip-weakening distance, so the distance between the two contours indicates cohesive zone width. The rupture follows areas of high initial shear traction, and is slowed where it enters low traction areas, causing focusing of the rupture front in some cases.

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[QuickTime movie]
5 MB

Movie 2: Surface Waves

Animation of surface velocity magnitude over three minutes of simulation time. Yellow indicates stronger velocities, exceeding 25 cm/s. Shock fronts due to super-shear rupture velocity are visible north of Palm Springs at around 45 seconds. Channeling of energy in to the basin wave guide near San Bernardino begins at about 60 seconds. Basin reverberations last well after the initial wave front has past, and are still present at the end of the simulation.

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[QuickTime movie]
10 MB