Seismic Anisotropy Analysis Across Southwestern Australia Reveals ENE-Trending Lithospheric Architecture Linked to Archean Yilgarn Craton Formation
| dc.contributor.author | Gauntlett, M. | en |
| dc.contributor.author | Eakin, C. M. | en |
| dc.contributor.author | Bishoyi, N. | en |
| dc.contributor.author | Zhang, P. | en |
| dc.contributor.author | O’Donnell, J. P. | en |
| dc.contributor.author | Murdie, R. E. | en |
| dc.contributor.author | Miller, M. S. | en |
| dc.contributor.author | Pickle, R. | en |
| dc.contributor.author | Ebrahimi, R. | en |
| dc.date.accessioned | 2026-02-26T06:40:49Z | |
| dc.date.available | 2026-02-26T06:40:49Z | |
| dc.date.issued | 2025 | en |
| dc.description.abstract | The southwest region of Western Australia is one of the oldest continental regions on Earth, hosting the Archean Yilgarn Craton, bounded by the Proterozoic Albany-Fraser and Pinjarra orogens. Here we calculate shear wave splitting of the PKS and SKS teleseismic phases using new broadband arrays with unprecedented station spacing across the region. We find evidence for coherent seismic anisotropy, with the regional average delay time ((Formula presented.) s) comparable to the global average, (Formula presented.) t = 1 s. Although fast polarization orientations show variation, they are not aligned with current plate motion and the expected mantle flow direction. In the South West Terrane and Albany-Fraser Orogen, fast polarization orientations match the trend of ancient structural faults. In contrast, structural faults in the Youanmi Terrane are oriented at an angle compared to the E–W and NE–SW fast polarizations. Instead, seismic anisotropy patterns show an intriguing similarity to E–W trending Precambrian (2.42 Ga) dykes that extend uninterrupted across the Yilgarn Craton. We propose that lithospheric fabrics frozen-in at the time of craton formation (2.76–2.65 Ga) generated a mechanical weakness which subsequently influenced the orientation and emplacement of the dykes. Further evidence for a similar, ancient (2.73 Ga) architectural fabric comes from recent isotope geochemistry analysis of primary ENE-trends within the Yilgarn Craton. Overall, these results point toward large-scale, fossilized lithospheric fabric within the Yilgarn Craton, preserved for over two billion years, offering a unique window into the formation and early evolution of the continent. | en |
| dc.description.sponsorship | We acknowledge that the seismic data used in this study were collected on the unceded sovereign Country of the Noongar, Badima, and Marlinyu Ghoorlie peoples. We thank them for their custodianship of the land and pay our respects to elders past, present and emerging. We are grateful for the feedback from editor Sergei Lebedev, and for the comments and advice from Kelly Liu and an anonymous reviewer, which helped improve this manuscript. We thank Janneke de Laat for sharing files with us. Author MG acknowledges financial and research support from the Geological Survey of Western Australia (GSWA). GSWA acknowledges funding by the state government of Western Australia. Author NB acknowledges financial support from a Future Research Talent scholarship at the Australian National University (ANU). Authors JPOD, RM, and RE publish with permission from the Executive Director of GSWA. We are grateful to colleagues at GSWA and ANU for their hard work in planning and carrying out the fieldwork for the ongoing WA Array deployment and the SWAN deployment. The SWAN network project was supported by the Australian Research Council (ARC)‐funded “Enhanced 3D Seismic structure for Southwest Australia” Linkage Project Number LP180101118. This is WA Array contribution #4. AUS22 We acknowledge that the seismic data used in this study were collected on the unceded sovereign Country of the Noongar, Badima, and Marlinyu Ghoorlie peoples. We thank them for their custodianship of the land and pay our respects to elders past, present and emerging. We are grateful for the feedback from editor Sergei Lebedev, and for the comments and advice from Kelly Liu and an anonymous reviewer, which helped improve this manuscript. We thank Janneke de Laat for sharing AUS22 files with us. Author MG acknowledges financial and research support from the Geological Survey of Western Australia (GSWA). GSWA acknowledges funding by the state government of Western Australia. Author NB acknowledges financial support from a Future Research Talent scholarship at the Australian National University (ANU). Authors JPOD, RM, and RE publish with permission from the Executive Director of GSWA. We are grateful to colleagues at GSWA and ANU for their hard work in planning and carrying out the fieldwork for the ongoing WA Array deployment and the SWAN deployment. The SWAN network project was supported by the Australian Research Council (ARC)-funded “Enhanced 3D Seismic structure for Southwest Australia” Linkage Project Number LP180101118. This is WA Array contribution #4. | en |
| dc.description.status | Peer-reviewed | en |
| dc.format.extent | 16 | en |
| dc.identifier.issn | 1525-2027 | en |
| dc.identifier.other | ORCID:/0000-0002-8550-5256/work/206439372 | en |
| dc.identifier.other | ORCID:/0000-0001-9187-3138/work/206439979 | en |
| dc.identifier.other | ORCID:/0000-0002-1050-6385/work/206440290 | en |
| dc.identifier.scopus | 105024888138 | en |
| dc.identifier.uri | https://hdl.handle.net/1885/733806627 | |
| dc.language.iso | en | en |
| dc.provenance | This is an open access article under theterms of the Creative CommonsAttribution License, which permits use,distribution and reproduction in anymedium, provided the original work isproperly cited | en |
| dc.rights | © 2025 The Author(s). | en |
| dc.source | Geochemistry, Geophysics, Geosystems | en |
| dc.subject | cratons | en |
| dc.subject | lithospheric structure | en |
| dc.subject | seismic anisotropy | en |
| dc.subject | shear wave splitting | en |
| dc.subject | Western Australia | en |
| dc.title | Seismic Anisotropy Analysis Across Southwestern Australia Reveals ENE-Trending Lithospheric Architecture Linked to Archean Yilgarn Craton Formation | en |
| dc.type | Journal article | en |
| dspace.entity.type | Publication | en |
| local.contributor.affiliation | Gauntlett, M.; Geophysics, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Eakin, C. M.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Bishoyi, N.; Australian National University | en |
| local.contributor.affiliation | Zhang, P.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | O’Donnell, J. P.; Geological Survey of Western Australia | en |
| local.contributor.affiliation | Murdie, R. E.; Geological Survey of Western Australia | en |
| local.contributor.affiliation | Miller, M. S.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Pickle, R.; Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.contributor.affiliation | Ebrahimi, R.; Geological Survey of Western Australia | en |
| local.identifier.citationvolume | 26 | en |
| local.identifier.doi | 10.1029/2025GC012589 | en |
| local.identifier.pure | 366dd72f-f1e4-4d67-89b4-4279d1d65712 | en |
| local.identifier.url | https://www.scopus.com/pages/publications/105024888138 | en |
| local.type.status | Published | en |
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