Xiaohan Song

and 3 more

Deep learning models have been widely applied in seismological signal processing, including phase picking, signal denoising, polarity determination, and phase association. But when it comes to the tasks to process phase information across a station network, most current workflows rely on either traditional physics informed optimization (e.g., hypocenter and grid search for source locations and focal mechanisms), or machine leaning models pre-trained on fixed station arrays, which limits the generality of the model to specific areas. We propose that by making proper use of transformer encoders (self-attention layers), in which we treat every station’s phase information as a “token vector” and append with the station locations/metadata as “positional encodings”, we can train a model capable of processing phase information from any general set of station networks.To demonstrate this idea, we built a transformer-based focal-mechanism determination model, named FOCONET, which directly solves for the strike, dip, and rake angles of a double couple focal mechanism, based on the locations, first-motion polarities, S/P amplitude ratios, and SNRs from a set of stations. FOCONET is trained on 440,000 noise-added synthetics generated with random source locations, focal mechanisms, and station distributions. We use the Kagan angle - the minimum rotation angle between the predicted and the (known) ground truth mechanism - to evaluate the prediction quality. Tested on the noised synthetics with known focal mechanisms, FOCONET reaches average Kagan angles of 29°, 16° and 12° when using data from 12, 24 or 32 stations. This is well within typical focal mechanism errors (25°–30°), and 3­º–10° lower than the predictions from traditional methods including: FPFIT and HASH (S/P included or excluded). We also tested our FOCONET on 200+ M>2.5 events of the 2016 Amatrice, Italy earthquake sequence with A-class HASH solutions for comparison, and achieved an average Kagan angle of 20º. Given its stronger performance on the synthetic test data, it is plausible that the FOCONET predictions may in fact be closer to the unknown ground truths. The success of FOCONET in focal mechanism determination from a network of stations suggests that similar joint-station seismological task would benefit from transformer-based models.
Understanding mechanical processes occurring on faults requires detailed information on the microseismicity that can be enhanced today by advanced techniques for earthquake detection. This problem is challenging when the seismicity rate is low and most of the earthquakes occur at depth. In this study, we compare three detection techniques, the autocorrelation FAST, the machine learning EQTransformer, and the template matching EQCorrScan, to assess their ability to improve catalogs associated with seismic sequences in the normal fault system of Southern Apennines (Italy) using data from the Irpinia Near Fault Observatory (INFO). We found that the integration of the machine learning and template matching detectors, the former providing templates for the cross-correlation, largely outperforms techniques based on autocorrelation and machine learning alone, featuring an enrichment of the automatic and manual catalogs of factors 21 and 7 respectively. Since output catalogs can be polluted by many false positives, we applied refined event selection based on the cumulative distribution of their similarity level. We can thus clean up the detection lists and analyze final subsets dominated by real events. The magnitude of completeness decreases by more than one unit compared to the reference value for the network. We report b-values associated with sequences smaller than the average, likely corresponding to larger differential stresses than for the background seismicity of the area. For all the analyzed sequences, we found that main events are anticipated by foreshocks, indicating a possible preparation process for mainshocks at sub-kilometric scales.

Xin Liu

and 1 more

Xin Liu

and 2 more

Cross-correlation of fully diffuse wavefields averaged over time should converge to the Green’s function; however, the ambient seismic field in the real Earth is not fully diffuse, which interferes with that convergence. We apply blind signal separation to reduce the effect of spurious non-diffuse components on the cross-correlation tensor of the ambient seismic field. We describe the diffuse component as having uncorrelated neighboring frequencies and equal intensity at all azimuths, and an independent (i.e., statistically uncorrelated) non-diffuse component arising from a spatially isolated point source for which neighboring frequencies are correlated. Under the assumption of linear independence of the spurious non-diffuse wave outside the stationary phase zone and the constructive interference of noise waves within that zone, we can suppress the spurious non-diffuse component from the noise interferometry. Our numerical simulations show good separation of one spurious non-diffuse noise source component for either non-diffuse Rayleigh or Love waves. We apply this separation to the Rayleigh-wave component of the Green’s function for 136 cross-correlation pairs from 17 stations in Southern California. We perform beamforming over different frequency bands for the cross-correlations before and after the separation, and find that the reconstructed Rayleigh waves are more coherent. We also estimate the bias in Rayleigh wave phase velocity for each receiver pair due to the spurious non-diffuse contribution.