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Annual Meeting - SCEC.org

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Group 2 – Tectonic Geodesy | Poster Abstracts<br />

2-002<br />

TESTING COMMUNITY VELOCITY MODELS FOR SOUTHERN CALIFORNIA<br />

USING THE AMBIENT SEISMIC FIELD Ma S, Prieto GA, and Beroza GC<br />

We correlate the vertical component of ambient seismic noise data recorded on 56 broadband<br />

stations with dense coverage in the greater Los Angeles area, to determine station-to-station<br />

Green’s functions. These Green’s functions provide an important test of community velocity<br />

models (<strong>SCEC</strong> CVM 4.0 and CVM-H 5.2) used for strong ground motion prediction for future<br />

scenario earthquakes in southern California. Comparisons of the ambient-noise Green’s functions<br />

for nearly 300 paths, with those calculated by the finite-element method in the community velocity<br />

models reveal a strong waveform similarity for the dominant surface waves between 0.1 and 0.2<br />

Hz. We find a mean correlation coefficient between the ambient-noise and finite-element Green’s<br />

functions of 0.62 for the CVM 4.0 and 0.49 for the CVM-H 5.2, indicating stronger waveform<br />

similarity for CVM 4.0. We also find that for 77% of the paths, the surface waves in the finiteelement<br />

Greens’ functions for CVM 4.0 arrive early, suggesting that the CVM 4.0 has velocities in<br />

the upper 10 km that are too fast along these paths. The same bias is evident for CVM-H 5.2, but is<br />

substantially smaller, with only 61% of the paths too fast. For 67% of the paths CVM 4.0 has<br />

velocities faster than CVM-H 5.2. The time lags we obtain between the ambient-noise and finiteelement<br />

Green’s functions provide key information for improving future community velocity<br />

models.<br />

2-003<br />

RESOLVING 3D FAULT GEOMETRY AT DEPTH ALONG ACTIVE STRIKE-SLIP<br />

FAULTS: SIMPLE OR COMPLEX? Nicholson C, Hauksson E, Plesch A, and Shearer PM<br />

A primary concern for <strong>SCEC</strong> in terms of understanding earthquake rupture and seismic hazard is<br />

resolving active 3D fault geometry at seismogenic depths. This is particularly important for<br />

properly extrapolating near-surface observations to depth where principal ruptures occur. This<br />

collaborative project is using recently developed seismicity and focal mechanism catalogs to<br />

identify the geometry and sense of slip of active fault segments at depth, and to help evaluate the<br />

<strong>SCEC</strong> Community Fault Model (CFM). This comparison forms the basis for identifying and<br />

developing improved fault representations for CFM, as well as identifying possible systematic<br />

biases in hypocentral location or fault models. In several places, aligned hypocenters are<br />

systematically offset from CFM 3D fault surfaces. This offset could be the result of: a) incorrect<br />

extrapolation of mapped surface fault traces to depth; b) earthquake mislocation owing to velocity<br />

models or location procedures used; or possibly c) existence of previously unidentified active<br />

subparallel fault strands. Along the Elsinore fault, active fault segments exhibit dips that vary<br />

along strike from about 80°SW to near-vertical to 70°NE. However, in CFM this fault is presumed<br />

to be vertical. Similar changes in dip along strike are found for the adjacent Agua Tibia-Earthquake<br />

Valley fault. Where the Elsinore fault is multi-stranded, fault segments separated by only a few<br />

kilometers can either remain subparallel throughout the seismogenic zone, or merge at depth to<br />

form y-shaped structures and intervening half-grabens, as appears to be the case beneath Lake<br />

Elsinore. Farther north, where the fault zone splays to form the Whittier and Chino faults, the<br />

seismicity exhibits a more complex 3D fault structure that includes intersecting high- and lowangle<br />

faults, as reflected in the recent 2008 Chino Hills earthquake sequence. At issue is whether<br />

these complex fault geometries defined by the microearthquakes are necessarily representative of<br />

the primary, through-going strike-slip fault that will likely produce the major slip and seismic<br />

moment release, or whether these structures illuminated by the seismicity only represent adjacent<br />

secondary faults. This issue is particularly important along the San Andreas fault, where various<br />

sections are largely aseismic and where models of the fault geometry at depth--being either<br />

2008 <strong>SCEC</strong> <strong>Annual</strong> <strong>Meeting</strong> | 143

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