週四, 24 十月 2013 15:27

[演講]Application of Seismic Array Back-Projection to Earthquake Early Warning

Invited Talk
Speaker:孟 令森博士 
Earthquake Physics Postdoc Fellow
Berkeley Seismo Lab
University of California-Berkeley

Title:Application of Seismic Array Back-Projection to Earthquake Early Warning 

Earthquake early warning (EEW) systems that can issue warnings prior to the arrival of strong ground shaking during an earthquake are essential in mitigating seismic hazard. Many of the currently operating EEW systems work on the basis of empirical magnitude-amplitude/frequency scaling relations for a point source. This approach is of limited effectiveness for large events, such as the 2011 Tohoku-Oki earthquake, for which ignoring finite source effects may result in underestimation of the magnitude. Here, we explore the concept of characterizing rupture dimensions in real time for EEW using clusters of dense low-cost accelerometers located near active faults. Back tracing the waveforms recorded by such arrays allows the estimation of the earthquake rupture size, duration and directivity in real-time, which enables the EEW of M > 7 earthquakes. The concept is demonstrated with the 2004 Parkfield earthquake, one of the few big events (M>6) that have been recorded by a local small-scale seismic array (UPSAR array, Fletcher et al, 2006). We first test the approach against synthetic rupture scenarios constructed by superposition of empirical Green's functions. We find it important to correct for the bias in back azimuth induced by dipping structures beneath the array. We implemented the proposed methodology to the mainshock in a simulated real-time environment. After calibrating the dipping-layer effect with data from smaller events, we obtained an estimated rupture length of 9 km, consistent with the distance between the two main high frequency subevents identified by back-projection using all local stations (Allman and Shearer, 2007). We proposed to deploy small-scale arrays every 30 km along the San Andreas Fault. The array processing is performed in local processing centers at each array. The output is compared with finite fault solutions based on real-time GPS system and then incorporated into the standard ElarmS system. The optimal aperture and array geometry is also investigated by balancing the array waveform coherency and resolution limits. The cost of such system can be significantly reduced by using recently developed low-cost accelerometers.

Time : 12:30 p.m. - 1:30 p.m., Tuesday, Oct. 29, 2013
Location :  Room 213, Department of Geosciences