Directivity Modes of Earthquake Populations with Unsupervised Learning
Abstract
We present a novel approach for resolving modes of rupture directivity in large populations of earthquakes. A seismic spectral decomposition technique is used to first produce relative measurements of radiated energy for earthquakes in a spatially compact cluster. The azimuthal distribution of energy for each earthquake is then assumed to result from one of several distinct modes of rupture propagation. Rather than fitting a kinematic rupture model to determine the most likely mode of rupture propagation, we instead treat the modes as latent variables and learn them with a Gaussian mixture model. The mixture model simultaneously determines the number of events that best identify with each mode. The technique is demonstrated on four datasets in California, each with compact clusters of several thousand earthquakes with comparable slip mechanisms. We show that the datasets naturally decompose into distinct rupture propagation modes that correspond to different rupture directions, and the fault plane is unambiguously identified for all cases. We find that these small earthquakes exhibit unilateral ruptures 63–73% of the time on average. The results provide important observational constraints on the physics of earthquakes and faults.
Additional Information
© 2020 American Geophysical Union. Received 1 JUL 2019; Accepted 31 JAN 2020; Accepted article online 5 FEB 2020. We thank Valère Lambert for helpful discussions. The waveform and catalog data used in this study are publicly available from the Southern California Earthquake Data Center (scedc.caltech.edu) and the Northern California Earthquake Data Center (ncedc.org). D. Trugman acknowledges institutional support from the Laboratory Directed Research and Development (LDRD) program of Los Alamos National Laboratory under project number 20180700PRD1. A. Anandkumar is supported in part by Bren endowed chair, Darpa PAI, Raytheon, and Microsoft, Google, and Adobe faculty fellowships. K. Azizzadenesheli is supported in part by NSF Career Award CCF‐1254106 and AFOSR YIPFA9550‐15‐1‐0221.Attached Files
Published - 2019JB018299.pdf
Submitted - 1907.00496.pdf
Supplemental Material - jgrb54024-sup-0001-2019jb018299-text_si-s01.pdf
Supplemental Material - jgrb54024-sup-0002-2019jb018299-data_set_si-s01.txt
Supplemental Material - jgrb54024-sup-0003-2019jb018299-data_set_si-s02.txt
Supplemental Material - jgrb54024-sup-0004-2019jb018299-data_set_si-s03.txt
Supplemental Material - jgrb54024-sup-0005-2019jb018299-data_set_si-s04.txt
Supplemental Material - jgrb54024-sup-0006-2019jb018299-data_set_si-s05.txt
Supplemental Material - jgrb54024-sup-0007-2019jb018299-data_set_si-s06.txt
Supplemental Material - jgrb54024-sup-0008-2019jb018299-data_set_si-s07.txt
Supplemental Material - jgrb54024-sup-0009-2019jb018299-data_set_si-s08.txt
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Additional details
- Eprint ID
- 98453
- Resolver ID
- CaltechAUTHORS:20190905-154247884
- Los Alamos National Laboratory
- 20180700PRD1
- Bren Professor of Computing and Mathematical Sciences
- Defense Advanced Research Projects Agency (DARPA)
- Raytheon
- Microsoft Faculty Fellowship
- Google Faculty Research Award
- Adobe
- NSF
- CCF‐1254106
- Air Force Office of Scientific Research (AFOSR)
- YIPFA9550‐15‐1‐0221
- Created
-
2019-09-05Created from EPrint's datestamp field
- Updated
-
2022-12-23Created from EPrint's last_modified field
- Caltech groups
- Seismological Laboratory, Division of Geological and Planetary Sciences (GPS)