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Testing the limits of virtual deep seismic sounding via new crustal thickness estimates of the Australian continent

dc.contributor.authorThompson, David A.
dc.contributor.authorRawlinson, Nicholas
dc.contributor.authorTkalčić, Hrvoje
dc.date.accessioned2020-03-05T00:40:38Z
dc.date.available2020-03-05T00:40:38Z
dc.date.issued2019
dc.date.updated2019-11-25T07:39:14Z
dc.description.abstractWe apply virtual deep seismic sounding (VDSS) to data collected from both permanent and temporary seismic stations in Australia with the goal of examining (i) the resilience of the method to the presence of complex lithospheric structure and (ii) the effectiveness of different approaches for estimating bulk crustal properties (namely thickness and Vp). Data from the permanent station WRAB in the Northern Territory is ideal for benchmarking VDSS (large number and favourable distribution of recorded earthquakes), with the results from several approaches agreeing on a thickness of 40–42 km. Application of VDSS to data from the temporary BILBY array, a linear distribution of broadband stations that traverses central Australia, shows that strong Moho reflections can be retrieved with as few as two earthquakes even at the transition between crustal blocks of different character and in the presence of thick sedimentary basins. Crustal thickness varies between 36 and 54 km and compares well with the reflectivity character of nearby deep seismic reflection lines. Furthermore, we find that off-line estimates of crustal thickness, calculated by binning the source regions according to back-azimuth, produce values of crustal thickness that are consistent with the regional geology. Overall, we find that VDSS is a powerful technique for estimating crustal thickness and velocity due to its insensitivity to complex short-wavelength structure and requirement of a small number earthquakes to produce a stable result. However, not all schemes tested for extracting bulk crustal properties appear to be robust and stringent data quality checking is still required during implementation.
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0956-540Xen_AU
dc.identifier.urihttp://hdl.handle.net/1885/202052
dc.language.isoen_AUen_AU
dc.provenancehttp://sherpa.ac.uk/romeo/issn/0956-540X/..."Publisher's version/PDF on Institutional repositories or Central repositories, with all rights reserved (see policy)" from SHERPA/RoMEO site (as at 05/03/2020). This article has been accepted for publication in Geophysical Journal International ©: The Author(s) 2019 Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.en_AU
dc.publisherOxford University Pressen_AU
dc.rights© The Author(s) 2019. Published by Oxford University Press on behalf of The Royal Astronomical Societyen_AU
dc.sourceGeophysical Journal Internationalen_AU
dc.titleTesting the limits of virtual deep seismic sounding via new crustal thickness estimates of the Australian continenten_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue2en_AU
local.bibliographicCitation.lastpage800en_AU
local.bibliographicCitation.startpage797en_AU
local.contributor.affiliationThompson, David A., Cardiff Universityen_AU
local.contributor.affiliationRawlinson, Nicholas, University of Aberdeenen_AU
local.contributor.affiliationTkalcic, Hrvoje, College of Science, ANUen_AU
local.contributor.authoruidTkalcic, Hrvoje, u4421436en_AU
local.description.notesImported from ARIES
local.identifier.absfor040407 - Seismology and Seismic Explorationen_AU
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciencesen_AU
local.identifier.ariespublicationu3102795xPUB3602en_AU
local.identifier.citationvolume218en_AU
local.identifier.doi10.1093/gji/ggz191en_AU
local.identifier.scopusID2-s2.0-85068553440
local.publisher.urlhttp://www.oxfordjournals.org/en_AU
local.type.statusPublished Versionen_AU

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