On the global centroid moment tensor achievements and the next generation earthquake catalogs

dc.contributor.authorPhạm, T. S.en
dc.contributor.authorTkalčić, H.en
dc.contributor.authorHu, J.en
dc.contributor.authorWei, Z.en
dc.date.accessioned2026-01-21T18:41:24Z
dc.date.available2026-01-21T18:41:24Z
dc.date.issued2026en
dc.description.abstractThe systematic determination of the source characteristics of global earthquakes and other seismic sources in a robust and consistent manner is a paramount task in seismology. The Global Centroid Moment Tensor (GCMT) project (Ekström et al., 2012), employing an elegant inversion approach and thoughtful data selection, has been a standard bearer for such an autonomous earthquake catalog. This, by no means an all-encompassing review, celebrates the long-lasting impact and legacy it has left on the seismological and broader Earth science community, from tectonics and structural geology to geodesy and hazard assessment. We also identify and discuss three areas that, in our view, are subject to potential improvement in the current GCMT practice. These include (i) enhanced quantification of uncertainty in MT solutions, (ii) utilization of 3D Earth models, and (iii) robust development of dynamic models that extend beyond a point source assumption in time and space. Recent developments in various areas of theoretical and observational seismology, such as advances in Bayesian inversion, 3D waveform modeling, and applied machine learning methods, will enable the integration of these needed elements into the next generation of routine earthquake catalogs.en
dc.description.sponsorshipT.-S. P. and H. T. acknowledge financial support from the Australian Research Council through a Discovery Early Career Research Award (DE230100025) and a Discovery Proposal (DP140102533). Additionally, H. T. is grateful for continuing support for seismic source studies through the US DoD/DoE and AFRL competitive Broad Agency Announcement schemes. We acknowledge computational support by the National Computational Infrastructure.en
dc.description.statusPeer-revieweden
dc.format.extent15en
dc.identifier.issn0031-9201en
dc.identifier.otherORCID:/0000-0001-7072-490X/work/202849426en
dc.identifier.otherORCID:/0000-0002-9057-4416/work/202850301en
dc.identifier.scopus105025553944en
dc.identifier.urihttps://hdl.handle.net/1885/733804784
dc.language.isoenen
dc.provenanceThis is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/).en
dc.rights © 2025 The Author(s)en
dc.sourcePhysics of the Earth and Planetary Interiorsen
dc.subjectCentroid moment tensoren
dc.subjectEarth modelen
dc.subjectInversionen
dc.subjectSource time functionen
dc.subjectUncertainty quantificationen
dc.titleOn the global centroid moment tensor achievements and the next generation earthquake catalogsen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.contributor.affiliationPhạm, T. S.; Geophysics, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationTkalčić, H.; Geophysics, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationHu, J.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationWei, Z.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume370en
local.identifier.doi10.1016/j.pepi.2025.107490en
local.identifier.puree621b48c-64f3-4d57-a457-3abd80f80b7cen
local.identifier.urlhttps://www.scopus.com/pages/publications/105025553944en
local.type.statusPublisheden

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