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Annual Meeting - SCEC.org

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Group 1 – GMP | Poster Abstracts<br />

Wald & Allen (2007). Our measurements were taken at 509 sites in California and Nevada. Most of<br />

the southern California measurements (188 sites) were taken along the San Gabriel River (Thelen et<br />

al., 2006) and were used by Wald & Allen (2007) in their regressions. An additional 96 sites were<br />

measured as a part of smaller studies in other parts of California. In Nevada, 109 sites were<br />

measured in the Reno basin affected by fluvial, alluvial, lacustrine, and tectonically-driven<br />

processes. On the basis of our Reno observations, the low correlation between Vs30 and slope we<br />

interpret to be influenced by the complexity of landscape evolution and less by topographic slope<br />

alone. Measurements in southern Nevada (116 sites) were influenced by the caliche development<br />

that dominates local soil development. Here, higher velocities are observed where topographic<br />

slope is lowest, contrary to the Wald & Allen (2007) model. Our analysis finds that 67% of our Vs30<br />

measurements (338 of 509) lie outside ±20% of the predicted values based on topographic slope.<br />

The RMS topographic prediction error is 161 m/s, or 45% of the measured Vs30. These results<br />

suggest that the Wald & Allen (2007) first-order approach based on slope is not able to reliably<br />

predict measured Vs30 values in regions of complex geology. Our results also highlight the<br />

inherent variability of shallow shear-wave velocity in complex environments and the need for<br />

more detailed Vs30 measurements to determine more refined predictive methods for<br />

microzonation.<br />

1-053<br />

CALCULATING THE SOURCE SENSITIVITY OF BASIN GUIDED WAVES BY TIME-<br />

REVERSED SIMULATIONS Day SM, Roten D, and Olsen KB<br />

Simulations of earthquake rupture on the southern San Andreas fault (e.g., TeraShake; ShakeOut)<br />

reveal large amplifications associated with channeling of seismic energy along contiguous<br />

sedimentary basins. Geometrically similar excitation patterns can be recognized repeatedly in<br />

different SAF simulations (e.g., Love wave-like energy with predominant period around 4 seconds,<br />

channeled southwestwardly from the San Gabriel basin into Los Angeles basin), yet the amplitudes<br />

with which these distinct wavefield patterns are excited differ, depending upon source details (slip<br />

distribution, direction and velocity of rupture).<br />

To improve understanding of the excitation of the high-amplitude patterns, we propose a<br />

numerical method for determining the sensitivity of a given wavefield pattern (i.e., one identified<br />

in a simulation, such as the above-cited sedimentary channeling effect identified in the ShakeOut<br />

simulations) to perturbations of the source kinematics. We first define a functional (phi(u), where u<br />

is the wavefield perturbation) that isolates the wavefield feature of interest and is proportional to<br />

its level of excitation. We then calculate the pullback of that functional onto the source by means of<br />

a single time-reversed (i.e., adjoint) simulation. The resulting functional (G*phi) now acts on the<br />

space of sources (slip functions) rather than wavefields, so given any source perturbation, we can<br />

calculate the resulting feature excitation without actually doing any forward wavefield<br />

simulations. In practice, the kernel of the pulled-back functional G*phi itself gives much insight<br />

into the feature-excitation sensitivity, and the time-reversal simulation itself helps ellucidate the<br />

wave propagation process leading to the wavefield feature in question.<br />

We applied this method to analyze the source sensitivity of the San Gabriel/Los Angeles channeled<br />

wave seen in ShakeOut simulations, finding: (i) Excitation is relatively insensitive to slip on the<br />

southernmost ~60 km long segment of the SAF (between Bombay Beach and Indio). (ii) Excitation<br />

is highly sensitive to slip on the ~100 km long SAF segment between Indio and San Bernardino, but<br />

only when the rupture is toward the NW, and especially when rupture velocity is near the<br />

maximum S wavespeed. (iii) Excitation is very insensitive to slip on the SAF north of San<br />

2008 <strong>SCEC</strong> <strong>Annual</strong> <strong>Meeting</strong> | 97

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