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dc.date.accessioned2018-08-14T16:15:15Z
dc.date.available2018-08-14T16:15:15Z
dc.date.created2018-01-29T15:59:07Z
dc.date.issued2017
dc.identifier.citationMaupin, Valerie . 3-D sensitivity kernels of the Rayleigh wave ellipticity. Geophysical Journal International. 2017, 211, 107-119
dc.identifier.urihttp://hdl.handle.net/10852/62961
dc.description.abstractThe ellipticity of the Rayleigh wave at the surface depends on the seismic structure beneath and in the vicinity of the seismological station where it is measured. We derive here the expression and compute the 3-D kernels that describe this dependence with respect to S-wave velocity, P-wave velocity and density. Near-field terms as well as coupling to Love waves are included in the expressions. We show that the ellipticity kernels are the difference between the amplitude kernels of the radial and vertical components of motion. They show maximum values close to the station, but with a complex pattern, even when smoothing in a finite-frequency range is used to remove the oscillatory pattern present in mono-frequency kernels. In order to follow the usual data processing flow, we also compute and analyse the kernels of the ellipticity averaged over incoming wave backazimuth. The kernel with respect to P-wave velocity has the simplest lateral variation and is in good agreement with commonly used 1-D kernels. The kernels with respect to S-wave velocity and density are more complex and we have not been able to find a good correlation between the 3-D and 1-D kernels. Although it is clear that the ellipticity is mostly sensitive to the structure within half-a-wavelength of the station, the complexity of the kernels within this zone prevents simple approximations like a depth dependence times a lateral variation to be useful in the inversion of the ellipticity.en_US
dc.languageEN
dc.publisherBlackwell Publishing
dc.title3-D sensitivity kernels of the Rayleigh wave ellipticityen_US
dc.typeJournal articleen_US
dc.creator.authorMaupin, Valerie
cristin.unitcode185,15,22,40
cristin.unitnameSenter for Jordens utvikling og dynamikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2
dc.identifier.cristin1555146
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical Journal International&rft.volume=211&rft.spage=107&rft.date=2017
dc.identifier.jtitleGeophysical Journal International
dc.identifier.volume211
dc.identifier.startpage107
dc.identifier.endpage119
dc.identifier.doihttp://dx.doi.org/10.1093/gji/ggx294
dc.identifier.urnURN:NBN:no-65499
dc.type.documentTidsskriftartikkelen_US
dc.type.peerreviewedPeer reviewed
dc.source.issn0956-540X
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/62961/2/Maupin_GJI2017.pdf
dc.type.versionPublishedVersion


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