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dc.contributor.authorXu, Shibo
dc.contributor.authorStovas, Alexey
dc.date.accessioned2019-01-05T09:50:18Z
dc.date.available2019-01-05T09:50:18Z
dc.date.created2018-09-24T11:42:28Z
dc.date.issued2017
dc.identifier.citationGeophysical Journal International. 2018, 213 (1), 181-193.nb_NO
dc.identifier.issn0956-540X
dc.identifier.urihttp://hdl.handle.net/11250/2579313
dc.description.abstractThe reflecting zone in the subsurface insonified by the first quarter of a wavelength and the portion of the reflecting surface involved in these reflections is called the Fresnel zone or first Fresnel zone. The horizontal resolution is controlled by acquisition factors and the size of the Fresnel zone. We derive an analytic expression for the radius of the Fresnel zone in time domain in transversely isotropic medium with a vertical symmetry axis (VTI) using the perturbation method from the parametric offset-traveltime equation. The acoustic assumption is used for simplification. The Shanks transform is applied to stabilize the convergence of approximation and to improve the accuracy. The similar strategy is applied for the azimuth-dependent radius of the Fresnel zone in orthorhombic (ORT) model for a horizontal layer. Different with the VTI case, the Fresnel zone in ORT model has a quasi-elliptic shape. We show that the size of the Fresnel zone is proportional to the corresponding traveltime, depth and the frequency. From the numerical examples, we can see that the Shanks transform approximations for Fresnel zone are very accurate for both VTI and ORT media.nb_NO
dc.language.isoengnb_NO
dc.publisherOxford University Pressnb_NO
dc.titleFreznel zone in VTI and orthorhombic medianb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionpublishedVersionnb_NO
dc.source.pagenumber181-193nb_NO
dc.source.volume213nb_NO
dc.source.journalGeophysical Journal Internationalnb_NO
dc.source.issue1nb_NO
dc.identifier.doi10.1093/gji/ggx544
dc.identifier.cristin1612884
dc.description.localcode© The Author(s) 2017. Published by Oxford University Press on behalf of The Royal Astronomical Society.nb_NO
cristin.unitcode194,64,90,0
cristin.unitnameInstitutt for geovitenskap og petroleum
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode2


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