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spelling ftinsu:oai:HAL:insu-02944202v1 2023-06-18T03:42:11+02:00 Stratification of the Earth beneath the Azores from P and S receiver functions Silveira, G. Vinnik, L. Stutzmann, E. Farra, V. Kiselev, S. Morais, I. Instituto Dom Luiz, Campo Grande, Edificio C8, 1749-016 Lisboa, Portugal Área Científica de Física, Instituto Superior de Engenharia de Lisboa, 1959-007 Lisboa, Portugal Institute of physics of the Earth, B. Grouzinskaya 10, 123995 Moscow, Russian Federation Institut de Physique du Globe de Paris (IPGP (UMR_7154)) Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) 2010-10 https://hal-insu.archives-ouvertes.fr/insu-02944202 https://doi.org/10.1016/j.epsl.2010.08.021 en eng HAL CCSD Elsevier info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2010.08.021 insu-02944202 https://hal-insu.archives-ouvertes.fr/insu-02944202 doi:10.1016/j.epsl.2010.08.021 ISSN: 0012-821X Earth and Planetary Science Letters https://hal-insu.archives-ouvertes.fr/insu-02944202 Earth and Planetary Science Letters, 2010, 299 (1-2), pp.91-103. ⟨10.1016/j.epsl.2010.08.021⟩ receiver functions hotspots mantle transition zone Azores [SDU]Sciences of the Universe [physics] info:eu-repo/semantics/article Journal articles 2010 ftinsu https://doi.org/10.1016/j.epsl.2010.08.021 2023-06-05T22:44:09Z International audience Seismic recordings of IRIS/IDA/GSN station CMLA and of several temporary stations in the Azores archipelago are processed with P and S receiver function (PRF and SRF) techniques. Contrary to regional seismic tomography these methods provide estimates of the absolute velocities and of the Vp/Vs ratio up to a depth of ~ 300 km. Joint inversion of PRFs and SRFs for a few data sets consistently reveals a division of the subsurface medium into four zones with a distinctly different Vp/Vs ratio: the crust ~ 20 km thick with a ratio of ~ 1.9 in the lower crust, the high-Vs mantle lid with a strongly reduced Vp/Vs velocity ratio relative to the standard 1.8, the low-velocity zone (LVZ) with a velocity ratio of ~ 2.0, and the underlying upper-mantle layer with a standard velocity ratio. Our estimates of crustal thickness greatly exceed previous estimates (~ 10 km). The base of the high-Vs lid (the Gutenberg discontinuity) is at a depth of ~ 80 km. The LVZ with a reduction of S velocity of ~ 15% relative to the standard (IASP91) model is terminated at a depth of ~ 200 km. The average thickness of the mantle transition zone (TZ) is evaluated from the time difference between the S410p and SKS660p, seismic phases that are robustly detected in the S and SKS receiver functions. This thickness is practically similar to the standard IASP91 value of 250 km, and is characteristic of a large region of the North Atlantic outside the Azores plateau. Our data are indicative of a reduction of the S-wave velocity of several percent relative to the standard velocity in a depth interval from 460 to 500 km. This reduction is found in the nearest vicinities of the Azores, in the region sampled by the PRFs, but, as evidenced by SRFs, it is missing at a distance of a few hundred kilometers from the islands. We speculate that this anomaly may correspond to the source of a plume which generated the Azores hotspot. Previously, a low S velocity in this depth range was found with SRF techniques beneath a few other hotspots. Article in Journal/Newspaper North Atlantic Institut national des sciences de l'Univers: HAL-INSU Ida ENVELOPE(170.483,170.483,-83.583,-83.583) Earth and Planetary Science Letters 299 1-2 91 103
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic receiver functions hotspots mantle transition zone Azores
[SDU]Sciences of the Universe [physics]
spellingShingle receiver functions hotspots mantle transition zone Azores
[SDU]Sciences of the Universe [physics]
Silveira, G.
Vinnik, L.
Stutzmann, E.
Farra, V.
Kiselev, S.
Morais, I.
Stratification of the Earth beneath the Azores from P and S receiver functions
topic_facet receiver functions hotspots mantle transition zone Azores
[SDU]Sciences of the Universe [physics]
description International audience Seismic recordings of IRIS/IDA/GSN station CMLA and of several temporary stations in the Azores archipelago are processed with P and S receiver function (PRF and SRF) techniques. Contrary to regional seismic tomography these methods provide estimates of the absolute velocities and of the Vp/Vs ratio up to a depth of ~ 300 km. Joint inversion of PRFs and SRFs for a few data sets consistently reveals a division of the subsurface medium into four zones with a distinctly different Vp/Vs ratio: the crust ~ 20 km thick with a ratio of ~ 1.9 in the lower crust, the high-Vs mantle lid with a strongly reduced Vp/Vs velocity ratio relative to the standard 1.8, the low-velocity zone (LVZ) with a velocity ratio of ~ 2.0, and the underlying upper-mantle layer with a standard velocity ratio. Our estimates of crustal thickness greatly exceed previous estimates (~ 10 km). The base of the high-Vs lid (the Gutenberg discontinuity) is at a depth of ~ 80 km. The LVZ with a reduction of S velocity of ~ 15% relative to the standard (IASP91) model is terminated at a depth of ~ 200 km. The average thickness of the mantle transition zone (TZ) is evaluated from the time difference between the S410p and SKS660p, seismic phases that are robustly detected in the S and SKS receiver functions. This thickness is practically similar to the standard IASP91 value of 250 km, and is characteristic of a large region of the North Atlantic outside the Azores plateau. Our data are indicative of a reduction of the S-wave velocity of several percent relative to the standard velocity in a depth interval from 460 to 500 km. This reduction is found in the nearest vicinities of the Azores, in the region sampled by the PRFs, but, as evidenced by SRFs, it is missing at a distance of a few hundred kilometers from the islands. We speculate that this anomaly may correspond to the source of a plume which generated the Azores hotspot. Previously, a low S velocity in this depth range was found with SRF techniques beneath a few other hotspots.
author2 Instituto Dom Luiz, Campo Grande, Edificio C8, 1749-016 Lisboa, Portugal
Área Científica de Física, Instituto Superior de Engenharia de Lisboa, 1959-007 Lisboa, Portugal
Institute of physics of the Earth, B. Grouzinskaya 10, 123995 Moscow, Russian Federation
Institut de Physique du Globe de Paris (IPGP (UMR_7154))
Institut national des sciences de l'Univers (INSU - CNRS)-Université de La Réunion (UR)-Institut de Physique du Globe de Paris (IPG Paris)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
format Article in Journal/Newspaper
author Silveira, G.
Vinnik, L.
Stutzmann, E.
Farra, V.
Kiselev, S.
Morais, I.
author_facet Silveira, G.
Vinnik, L.
Stutzmann, E.
Farra, V.
Kiselev, S.
Morais, I.
author_sort Silveira, G.
title Stratification of the Earth beneath the Azores from P and S receiver functions
title_short Stratification of the Earth beneath the Azores from P and S receiver functions
title_full Stratification of the Earth beneath the Azores from P and S receiver functions
title_fullStr Stratification of the Earth beneath the Azores from P and S receiver functions
title_full_unstemmed Stratification of the Earth beneath the Azores from P and S receiver functions
title_sort stratification of the earth beneath the azores from p and s receiver functions
publisher HAL CCSD
publishDate 2010
url https://hal-insu.archives-ouvertes.fr/insu-02944202
https://doi.org/10.1016/j.epsl.2010.08.021
long_lat ENVELOPE(170.483,170.483,-83.583,-83.583)
geographic Ida
geographic_facet Ida
genre North Atlantic
genre_facet North Atlantic
op_source ISSN: 0012-821X
Earth and Planetary Science Letters
https://hal-insu.archives-ouvertes.fr/insu-02944202
Earth and Planetary Science Letters, 2010, 299 (1-2), pp.91-103. ⟨10.1016/j.epsl.2010.08.021⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1016/j.epsl.2010.08.021
insu-02944202
https://hal-insu.archives-ouvertes.fr/insu-02944202
doi:10.1016/j.epsl.2010.08.021
op_doi https://doi.org/10.1016/j.epsl.2010.08.021
container_title Earth and Planetary Science Letters
container_volume 299
container_issue 1-2
container_start_page 91
op_container_end_page 103
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