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hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
dc.contributor.authorTRABATTONI, A.
hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
dc.contributor.authorBARRUOL, G.
hal.structure.identifierInstitut de Recherche de l'Ecole Navale [IRENAV]
dc.contributor.authorDREO, R
hal.structure.identifierInstitut de Recherche de l'Ecole Navale [IRENAV]
dc.contributor.authorBOUDRAA, A
hal.structure.identifierLaboratoire GéoSciences Réunion [LGSR]
hal.structure.identifierInstitut de Physique du Globe de Paris [IPGP]
dc.contributor.authorFONTAINE, Fabrice R.
dc.date.accessioned2021-05-14T09:38:00Z
dc.date.available2021-05-14T09:38:00Z
dc.date.created2020
dc.date.issued2020
dc.identifier.issn0956-540X
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/76396
dc.description.abstractEnBreakthroughs in understanding the structure and dynamics of our planet will strongly depend upon instrumenting deep oceans. Progress has been made these last decades in ocean-bottom seismic observations, but ocean-bottom seismometer (OBS) temporary deployments are still challenging and face setup limitations. Launched from oceanographic vessels, OBSs fall freely and may slightly drift laterally, dragged by currents. Therefore, their actual orientation and location on the landing sites are hard to assess precisely. Numerous techniques have been developed to retrieve this key information, but most of them are costly, time-consuming or inaccurate. In this work, we show how ship noise can be used as an acoustic source of opportunity to retrieve both the orientation and the location of OBSs on the ocean floor. To retrieve the OBS orientation, we developed a first method based on a combination of seismic and pressure data through the use of the acoustic intensity. This latter can be used to quantify the OBS orientation from the ship noise direction of arrival (DOA), which can then be compared with known ship trajectories obtained from the automatic identification system (AIS). To accurately relocate OBSs, we also developed a second method based on the hydrophone data which computes distances of acoustical sources by measuring time differences of arrival (TDOA) between direct and reverberated phases. The OBS location is then retrieved by fitting measured ship distances with known ship trajectories. In this study, a full network of OBSs deployed in the SW Indian Ocean was reoriented and a test station was relocated. We demonstrate that our new methods may quantify the OBS orientation with an accuracy of about one degree, and its location with an accuracy of a few tens of metres, depending on the number of ships used in the analysis.
dc.description.sponsorshipImagerie mantellique du point chaud de La Réunion - ANR-11-BS56-0013
dc.language.isoen
dc.publisherOxford University Press (OUP)
dc.subject.enSeismic noise
dc.subject.enWave propagation
dc.subject.enBody waves
dc.subject.enStatistical methods
dc.subject.enSeismic instruments
dc.subject.enAcoustic properties
dc.title.enOrienting and locating ocean-bottom seismometers from ship noise analysis
dc.typeArticle de revue
dc.identifier.doi10.1093/gji/ggz519
dc.subject.halPlanète et Univers [physics]/Sciences de la Terre/Géophysique [physics.geo-ph]
bordeaux.journalGeophysical Journal International
bordeaux.page1774-1790
bordeaux.volume220
bordeaux.hal.laboratoriesInstitut de Mécanique et d’Ingénierie de Bordeaux (I2M) - UMR 5295*
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionBordeaux INP
bordeaux.institutionCNRS
bordeaux.institutionINRAE
bordeaux.institutionArts et Métiers
bordeaux.peerReviewedoui
hal.identifierhal-02392669
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02392669v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Geophysical%20Journal%20International&rft.date=2020&rft.volume=220&rft.spage=1774-1790&rft.epage=1774-1790&rft.eissn=0956-540X&rft.issn=0956-540X&rft.au=TRABATTONI,%20A.&BARRUOL,%20G.&DREO,%20R&BOUDRAA,%20A&FONTAINE,%20Fabrice%20R.&rft.genre=article


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