Annual Meeting - SCEC.org
Annual Meeting - SCEC.org
Annual Meeting - SCEC.org
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Group 1 – ShakeOut | Poster Abstracts<br />
Attenuation (NGA) empirical relations very closely (i.e., within roughly their epistemic<br />
uncertainty) over the distance range 2-200 km, and intra-event standard deviations are very close<br />
to the empirical values over the distance range 0 and 50 km. The simulations predict entrainment<br />
by basin structure of a strong directivity pulse, with long-period spectral accelerations in Los<br />
Angeles and Ventura basins significantly larger than those predicted by the empirical relations.<br />
The ShakeOut-D ground motion predictions differ in some important respects from a recent<br />
kinematically parameterized simulation of a geometrically similar scenario: (1) the kinematic rocksite<br />
predictions depart significantly from the common distance-attenuation trend of the NGA and<br />
ShakeOut-D results, and (2) ShakeOut-D predictions of long-period spectral acceleration within the<br />
basins of the greater Los Angeles area, including those with concentrations of high-rise buildings,<br />
are lower by factors of 2-3 than the corresponding kinematic predictions. The latter result agrees<br />
with the results from a previous comparison of kinematically and dynamically parameterized<br />
simulations of Mw7.7 San Andreas scenarios (TeraShake). As in the previous study, we attribute<br />
the difference to reduced forward directivity due to the less coherent wavefield excited by the<br />
spontaneous-rupture sources.<br />
1-047<br />
IMPLICATIONS OF THE SHAKEOUT SOURCE DESCRIPTION FOR RUPTURE<br />
COMPLEXITY AND NEAR-SOURCE GROUND MOTION Dalguer LA, Day SM, Olsen KB,<br />
Cruz-Atienza VM, Cui Y, Zhu J, Gritz A, Okaya DA, and Maechling PJ<br />
With the goal to evaluate the implications of the source description of the SoSAFE ShakeOut<br />
scenario for the rupture and ground motion, we developed a diversity of large-scale dynamic<br />
models in the Southern San Andreas fault. Four classes of models are considered: Each of the first<br />
three classes incorporates stochastic irregularities in the stress drop compatible with seismological<br />
observations, combined with some degree of constraint on the long-wavelength component of slip:<br />
(i) Models that have stress drop preconditioned such that Mw and final surface slip approximate<br />
the corresponding moment and slip-profile (or background slip) distribution along the strike of the<br />
fault specified for ShakeOut by Hudnut et al. (2008). (ii) Models preconditioned so as to the depthaveraged<br />
slip matches the slip-profile specified by Hudnut et al. and such that they match Mw as<br />
well (iii). Models that match the ShakeOut Mw only. The constraints were imposed using a slipmatching<br />
technique that iteratively performs kinematic and dynamic rupture simulations to find<br />
stress drop distribution that yields the prescribed ShakeOut static slip characteristics. We also<br />
investigated a fourth class of model based on simple asperities following the rules proposed by<br />
Dalguer at al., 2008, BSSA, and matching only the fault dimensions of ShakeOut (notice that by<br />
simply using this rule, the Mw also approximates the ShakeOut Mw). The class (i) and class (ii)<br />
models each have two well-defined patches of high stress drop at the extremes of the fault,<br />
corresponding to the a priori slip constraints from the ShakeOut scenario. All the fault models are<br />
planar faults, and each dynamic model is the first step of a two-step procedure to calculate ground<br />
motion for the ShakeOut scenario (see the poster of Olsen et al). Here we examine the rupture<br />
complexity and the qualitative ground motion characteristics of these models, referring to the<br />
poster of Olsen et al. for quantitative details of the ground motion estimates. All the models<br />
generate the strongest ground motion next to the fault, driven mainly by deep patches of high<br />
stress drop. Qualitatively, we note that the class (iii) and (iv) models are apparently more efficient<br />
in exciting the San Gabriel and Los Angeles basin areas than are the slip-constrained class (i) and<br />
(ii) models, probably because the slip distribution imposed on the latter models is not optimal for<br />
exciting the guided-wave channel between San Andreas fault and Los Angeles basin.<br />
2008 <strong>SCEC</strong> <strong>Annual</strong> <strong>Meeting</strong> | 93