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dc.contributor.authorAyarza Arribas, María Puy 
dc.contributor.authorPalomeras Torres, Inmaculada 
dc.contributor.authorCarbonell, R.
dc.contributor.authorAfonso, J.C.
dc.contributor.authorSimancas, F.
dc.date.accessioned2024-02-07T09:57:55Z
dc.date.available2024-02-07T09:57:55Z
dc.date.issued2010
dc.identifier.citationP. Ayarza, I. Palomeras, R. Carbonell, J.C. Afonso, F. Simancas, A wide-angle upper mantle reflector in SW Iberia: Some constraints on its nature, Physics of the Earth and Planetary Interiors, Volume 181, Issues 3–4, 2010, Pages 88-102, ISSN 0031-9201, https://doi.org/10.1016/j.pepi.2010.05.004. (https://www.sciencedirect.com/science/article/pii/S0031920110001032)es_ES
dc.identifier.issn0031-9201
dc.identifier.urihttp://hdl.handle.net/10366/155469
dc.description.abstract[EN]Deep and fast wide-angle reflection arrivals observed at offsets over 180 km, and over a reduced time interval of 1–1.5 s, have been observed in a seismic experiment shot across SW Iberia as part of the IBERSEIS project. Using different modelling approaches, these reflections have been found to be consistent with a heterogeneous gradient zone located at 61–72 km depth that features an absolute P-wave velocity contrast from 8.2 to 8.3 km/s. Paradoxically, this interface has not been observed in coincident vertical incidence data, probably due to the change in the reflection coefficient with decreasing incidence angles, the lack of energy at high recording times for the near-vertical (vibroseis) data, and/or the different location of the CDPs in both experiments. Although the mantle is acknowledged to be highly heterogeneous and mantle lithologies are capable of giving impedance contrasts high enough as to be observed in seismic data, it is often seen as transparent from a seismic point of view. The short wavelength of mantle compositional heterogeneities is probably what hinders their identification with active source seismic data and only big and sharp discontinuities are imaged in vertical incidence experiments whereas regional transitional boundaries may be also observed at high incidence angles. Accordingly, we propose that deep reflectivity observed in SW Iberia must correspond to a regional–continental scale feature, not sharp enough as to be seen with vertical incidence energy. This feature, already identified in previous DSS experiments carried out in Iberia, has a depth, a P-wave velocity contrast and a transitional nature that match the characteristics proposed for the spinel-lherzolite to garnet-lherzolite phase transition, i.e. the Hales interface or gradient zone. This boundary is relatively narrow (at least 2–3 kb) in enriched mantle and appears deeper and along wider intervals when the mantle is depleted. In addition, it is a worldwide scale boundary already identified over large areas with different types of datasets. The variability in depth and sharpness of this interface, which is related to mantle chemistry, constrains the type of seismic techniques that should be used to identify it.es_ES
dc.format.mimetypeapplication/pdf
dc.language.isoenges_ES
dc.publisherElsevieres_ES
dc.subjectWide-angle seismic experiment IBERSEISes_ES
dc.subjectSW Iberia Variscan beltes_ES
dc.subjectUpper mantlees_ES
dc.subjectSpinel-lherzolite Garnet-lherzolitees_ES
dc.subjectHales gradient zonees_ES
dc.titleA wide-angle upper mantle reflector in SW Iberia: Some constraints on its nature.es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publishversionhttps://doi.org/10.1016/j.pepi.2010.05.004es_ES
dc.identifier.doi10.1016/j.pepi.2010.05.004
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.journal.titlePhysics of the Earth and Planetary Interiorses_ES
dc.volume.number181es_ES
dc.issue.number3-4es_ES
dc.page.initial88es_ES
dc.page.final102es_ES
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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