Project Abstract
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We discovered a new type of seismological signature, fault zone trapped noise (Hillers et al. 2014), that extends the range of previously known ballistic fault zone waves. Analyzing data from the Calico field experiment we studied the interaction of the ambient seismic wavefield with a fault zone environment; we showed that the high-frequency wavefield in the fault differs from the field in the adjacent crust. Noise within the fault is characterized by significantly increased isotropy, which indicates that randomization of propagation directions is more efficient, and energy can be considered as trapped. We showed that conditions controlling the emergence of seismic fault zone trapped noise have less limitations compared to trapped ballistic waves. We proposed to investigate the potential of the correlation field associated with trapped noise to provide a high resolution tool for imaging the internal structure (dimensions, seismic velocity, attenuation, continuity) of fault damage zones, in analogy to properties of fault zone trapped waves (e.g., Li et al., 1990, 1994; Ben-Zion et al., 2003; Lewis et al., 2005). We construct noise correlation functions from the scattered seismic wavefield recorded by a spatially dense array with >1100 vertical-component nodes centered on the Clark segment of the San Jacinto Fault Zone southeast of Anza (BenZion et al., 2015). Based on estimates of the similarity of causal and acausal waveforms we assess the noise correlation symmetry, which is an indicator of noise wavefield isotropy. Spatial distributions of similarity and hence isotropy markers can be indicative of trapping and waveguiding structures. |