Point source moment tensor inversion through a Bayesian hierarchical model
| dc.contributor.author | Mustać, Marija | |
| dc.contributor.author | Tkalčić, Hrvoje | |
| dc.date.accessioned | 2017-12-12T05:24:06Z | |
| dc.date.available | 2017-12-12T05:24:06Z | |
| dc.date.issued | 2015 | |
| dc.description.abstract | Characterization of seismic sources is an important aspect of seismology. Parameter uncertainties in such inversions are essential for estimating solution robustness, but are rarely available. We have developed a non-linear moment tensor inversion method in a probabilistic Bayesian framework that also accounts for noise in the data. The method is designed for point source inversion using waveform data of moderate-size earthquakes and explosions at regional distances. This probabilistic approach results in an ensemble of models, whose density is proportional to parameter probability distribution and quantifies parameter uncertainties. Furthermore, we invert for noise in the data, allowing it to determine the model complexity. We implement an empirical noise covariance matrix that accounts for interdependence of observational errors present in waveform data. After we demonstrate the feasibility of the approach on synthetic data, we apply it to a Long Valley Caldera, CA, earthquake with a well-documented anomalous (non-double-couple) radiation from previous studies. We confirm a statistically significant isotropic component in the source without a trade-off with the compensated linear vector dipoles component. | en_AU |
| dc.description.sponsorship | Marija Mustac was supported by an Australian National University ´ Research Scholarship and AE Ringwood Supplementary Scholarship. The research was also supported by the USA DoD/AFRL under grant no. FA9453-13-C-0268. | en_AU |
| dc.format.mimetype | application/pdf | en_AU |
| dc.identifier.issn | 0956-540X | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/138026 | |
| dc.publisher | Oxford University Press | en_AU |
| dc.rights | © The Authors 2015. Published by Oxford University Press on behalf of The Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the original work is properly cited. | en_AU |
| dc.source | Geophysical Journal International | en_AU |
| dc.subject | Time-series analysis | en_AU |
| dc.subject | Inverse theory | en_AU |
| dc.subject | Earthquake source observations | en_AU |
| dc.subject | Surface waves and free oscillations | en_AU |
| dc.subject | Computational seismology | en_AU |
| dc.title | Point source moment tensor inversion through a Bayesian hierarchical model | en_AU |
| dc.type | Journal article | en_AU |
| dcterms.accessRights | Open Access | en_AU |
| local.bibliographicCitation.issue | 1 | en_AU |
| local.bibliographicCitation.lastpage | 323 | en_AU |
| local.bibliographicCitation.startpage | 311 | en_AU |
| local.contributor.affiliation | Mustać, M., Research School of Earth Sciences, The Australian National University | en_AU |
| local.contributor.affiliation | Tkalčić, H., Research School of Earth Sciences, The Australian National University | en_AU |
| local.contributor.authoruid | u5095777 | en_AU |
| local.identifier.ariespublication | U3488905xPUB11575 | |
| local.identifier.citationvolume | 204 | en_AU |
| local.identifier.doi | 10.1093/gji/ggv458 | en_AU |
| local.publisher.url | https://academic.oup.com/journals/ | en_AU |
| local.type.status | Published Version | en_AU |