Receiver structure from teleseisms: autocorrelation and cross correlation
dc.contributor.author | Sun, Weijia | |
dc.contributor.author | Kennett, B. L. N. | |
dc.date.accessioned | 2017-01-03T23:33:02Z | |
dc.date.available | 2017-01-03T23:33:02Z | |
dc.date.issued | 2016-06-28 | |
dc.description.abstract | We present a way of characterizing the structure beneath a seismic station, by exploiting stacked correlograms of three-component records from teleseismic events. This seismic daylight imaging approach exploits the extraction of reflection and conversion information from teleseismic coda via tensor autocorrelation. The approach is illustrated for a number of Australian stations in a variety of tectonic environments using hundreds of teleseismic events, to extract P and S reflectivity and converted Ps and Sp information. The results show a very good agreement with prior knowledge across Australia. Compared with the classical receiver function, the broader-frequency band of 0.5–4.0 Hz provides additional information on finer-scale structure. | en_AU |
dc.description.sponsorship | The research was supported in large part by the State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences and the National Natural Science Foundation of China (grant 41474105), with additional support from the AuScope AuSREM project. | en_AU |
dc.format | 9 pages | en_AU |
dc.format.mimetype | application/pdf | en_AU |
dc.identifier.issn | 0094-8276 | en_AU |
dc.identifier.uri | http://hdl.handle.net/1885/111465 | |
dc.publisher | American Geophysical Union | en_AU |
dc.rights | ©2016. American Geophysical Union. http://publications.agu.org/author-resource-center/usage-permissions/ Not subject to U.S. copyright. (Publisher journal website 4/1/2017). http://www.sherpa.ac.uk/romeo/issn/0094-8276/ Author can archive publisher's version/PDF. Publisher's version/PDF must be used in Institutional Repository 6 months after publication. (Sherpa/Romeo as of 4/1/2017). | en_AU |
dc.source | Geophysical Research Letters | en_AU |
dc.subject | stacked | en_AU |
dc.subject | correlograms | en_AU |
dc.subject | teleseismic | en_AU |
dc.subject | events | en_AU |
dc.subject | seismic | en_AU |
dc.subject | daylight | en_AU |
dc.subject | imaging | en_AU |
dc.subject | reflection | en_AU |
dc.subject | conversion | en_AU |
dc.subject | tensor | en_AU |
dc.subject | autocorrelation | en_AU |
dc.subject | Australia | en_AU |
dc.subject | tectonic | en_AU |
dc.subject | environment | en_AU |
dc.title | Receiver structure from teleseisms: autocorrelation and cross correlation | en_AU |
dc.type | Journal article | en_AU |
dcterms.accessRights | Open Access | en_AU |
dcterms.dateAccepted | 2016-06-08 | |
local.bibliographicCitation.issue | 12 | en_AU |
local.bibliographicCitation.lastpage | 6242 | en_AU |
local.bibliographicCitation.startpage | 6234 | en_AU |
local.contributor.affiliation | Kennett, Brian L. N., RSES General, CPMS Research School of Earth Sciences, The Australian National University | en_AU |
local.contributor.authoremail | Brian.Kennett@anu.edu.au | en_AU |
local.contributor.authoruid | u8413736 | en_AU |
local.identifier.citationvolume | 43 | en_AU |
local.identifier.doi | 10.1002/2016GL069564 | en_AU |
local.identifier.essn | 1944-8007 | en_AU |
local.identifier.uidSubmittedBy | u4579722 | en_AU |
local.publisher.url | http://sites.agu.org/ | en_AU |
local.type.status | Published Version | en_AU |
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