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Ground Motions: 2004 Annual Report

The challenge facing the ground motion group is validation of codes against available data so that broadband ground motions relevant to building damage can be predicted with confidence from future earthquakes. While considerable progress has been made at frequencies below 1 Hz, large-scale high-frequency modeling is beyond both computational resources and our detailed knowledge of source and path. Various empirical schemes have been used to add high frequencies to computed seismograms, but without a physical basis their reliability is in question. Even at low frequencies, inadequate knowledge of the path limits how much of the coda can be predicted. Both high frequency strong shaking and long-term coda are important for engineering considerations. The ground motion group has made significant progress in attacking these problems with a series of numerical calculations, validations and experiments coordinated with other groups across SCEC (e.g., ESP, IIG, CVM, CFM, USR,CME).

Numerical Simulations

Larger imageTerashake movie frame. The rupture travels SE along the San Andreas fault. Note the directivity to the southeast, trapping of waves in the Los Angeles and Ventura basins and irregular shaking pattern from fault segmentation.

Probably the largest computation of ground motion to date was Terashake performed by the CME group using Kim Olsen’s finite difference program. The southern California region was divided into 1.8 billion 200m cubes, and seismograms up to 0.5 Hz were generated from a Denali-type earthquake rupturing 230 km of the San Andreas fault. The calculation ran for four days on the San Diego DataStar supercomputer and generated 47 Tbytes of data (surely one for the Guinness book of world records). The spectacular movies of surface ground motion were shown at the SCEC annual meeting with vivid depiction of effects of directivity, fault segmentation, scattering, trapping of basin waves and generation of long term coda.

A number of different methods have been implemented to model the high frequency part of seismograms. Yehua Zeng uses a combination of rough source, randomly distributed scatterers and reverberations in near surface layering. Arben Pitarka and Rob Graves add a stochastic component to low frequency deterministic calculations. Tom Heaton adds high frequency data from nearby strong motion instruments to wavefields calculated using Jeroen Tromp’s spectral element method. Kim Olsen uses finite differences to model low frequencies and ray synthetics to deterministically model high frequencies with sources constrained by pseudo dynamics. The method claims smoother phase transitions across the spectral band. The same source model is used and a weighted superposition is used to combine the low and high frequency bands. The optimal method continues to be an area of active enquiry.

The ground motion group were active participants in the PEER-USGS-SCEC sponsored NGA-E (Next Generation Attenuation) project that has now been funded directly by NSF for a 3-year project. The SCEC research involves comparison of broadband simulations against data from large earthquakes (See IIG report). The NGA modeling effort presents an essential conduit through which SCEC research flows to practical use.

Modeling and Observations

Larger imageFoam rubber simulations. The model is shown upper left. The data (red lines) is compared with Steve Day’s dynamic rupture code, which matches low frequencies but not the high frequencies generated on the fault plane.

The foam rubber test-bed in Jim Brune’s lab has been used to validate Steve Day’s dynamic rupture code. At low frequencies the comparison is excellent, but at high frequency the smooth numerical model does not capture the high amplitude accelerations that develop in the vicinity of the fault. This observation, also seen in earthquake records, is referred to as the roughness ratio, RR (high-f to low-f acceleration, RR~3). It suggests that, even in a nominally smooth physical model, the dynamics introduces rough behavior, possibly due to interface chatter, such as opening and closing modes, or dynamical effects causing variable friction. These observations reinforce the view that in order to understand high frequency ground motion it is critical to separate source and path effects. Comparisons between modeling and data have raised the following questions: (1) Why do the foam rubber models and numerical comparison over-predict directivity at high frequency in comparison with observations? (2) Why do they not exhibit along strike saturation; is this due to lack of asperities in rubber? (3) Why are high frequency accelerations several times low frequency accelerations? (4) Standard models find that spectral amplitudes increase with magnitude. However observations imply the near fault pulse is narrow band and period increases with magnitude. (5) Weaker ground motion is observed when faulting breaks the surface.

Work continues on finding geological constraints on historic strong ground motion by analyzing survivability of precariously balanced rocks. After the remarkable observation of a line of rocks mid-way between the Elsinore and San Jacinto faults, presumed to be located just far enough from each to survive historic shaking, a new reconnaissance study of the region between the San Andreas and San Jacinto is being undertaken. Further theoretical and observational work continues to quantify the observations.

Path and Scattering Effects

Kim Olsen introduced an empirical Q model into the CVM, where Q was taken to be proportional to S wave speed. This resulted in significant variance reduction between theory and data. Peter Shearer and Egill Haukkson are inferring Q from local earthquake data. They use stacked spectra from hundreds of thousands of double difference-relocated events to isolate source, path, and site spectral response. At the SCEC meeting they presented a new Q model for the upper crust. Jamie Steidl and Pengcheng Liu have inverted for Q(z,f) at various depths in the SCEC borehole seismic array, and show that at high frequencies the last few hundred meters can be as attenuative as the remaining path. Ralph Archuleta is examining source, path and site effects on the 150 station Yokahama seismic array with the objective of explaining long durations and the various ground motion factors relative to the geology.

Larger imageShear wave velocity cross sections through the SCEC and Harvard 3D velocity models (click for details...)

Larger imageMap of peak simulated ground velocity for the Northridge earthquake.

Rob Graves has compared Northridge earthquake synthetics from the SCEC velocity model and the Harvard velocity model. The models are generally similar in their representation of the basin structures. However, several key differences are apparent, particularly in the structure of the northern San Fernando basin. Both simulation models do reasonably well at reproducing the general characteristics (i.e., waveform and amplitude) of the observed time histories at these sites, with the exception of the Harvard model at sylm. The different simulation response at sylm is explained by the lack of basin structure at this site in the Harvard model. This work represents a start at reconciling the two models to arrive at an optimal CVM for ground motion predictions.

Engineering Applications

Tom Heaton leads an effort involving active collaboration between building and ground modelers to model the hazard presented by the newly discovered Puente Hills blind thrust. Ground motions up to 1.5 Hz are calculated using Tromp’s spectral elements program, coupled with historic recordings of strong ground motion for higher frequencies. Programs written by (structural engineer) Hall’s group have been used to model building response for (up to) 40- floor buildings. The simulations are used to identify times and locations of structural damage. The structure codes can take the buildings all the way to collapse. Various movies of building excitation were presented at the SCEC annual meeting with assessment of maximum damage presented in graphical form on the structural drawings.

Future Directions

Future directions include comparing and validating broadband ground motion with observations and improving modeling schemes; Testing of the CVM and inversion of observed seismograms to improve the CVM; Adding to the CVM the SCEC scattering and attenuation model by identifying and modeling sources of scattering; Developing methods for incorporating nonlinear site response for large amplitude ground motion events in Southern California including site and structural response; Developing collaborations with engineers (with IIG) to add building response to synthetic seismograms and identify seismogram characteristics important for damage.





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