Abstract
Highly damaged rocks within the San Andreas fault zone at Parkfield
form a low-velocity waveguide for seismic waves, giving rise to fault-guided
waves. Prominent fault-guided waves have been observed at the San
Andreas Fault Observatory at Depth (SAFOD) site, including a surface
array across the fault zone and a borehole seismograph placed in
the SAFOD well at a depth of \~2.7 km below ground. The resulting
observations are modeled here using 3-D finite-difference methods.
To fit the amplitude, frequency, and travel-time characteristics
of the data, the models require a downward tapering, 30-40-m wide
fault-core embedded in a 100-200-m wide jacket. Compared with the
intact wall rocks, the core velocities are reduced by \~40\% and
jacket velocities by \~25\%. Based on the depths of earthquakes
generating guided waves, we estimate that the low-velocity waveguide
along the fault at SAFOD extends at least to depths of \~7 km,
more than twice the depth reported in pervious studies.
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