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Title

3D tomographic imaging of the Cayman Trough lithosphere: challenges, ongoing work and first results

AuthorsGómez de la Peña, L. CSIC ORCID; Grevemeyer, Ingo; Dannowsky, Anke; Meléndez, Adrià CSIC ORCID ; Peirce, Christine; Avendonk, Harm van
Issue Date26-Apr-2021
PublisherEuropean Geosciences Union
CitationEuropean Geosciences Union General Assembly (2021)
AbstractAbout 25% of the Earth’s mid-ocean ridges spread at ultraslow rates of less than 20 mm/yr. However, most of these ultraslow spreading ridges are located in geographically remote areas, which hamper investigation. Consequently, how the crust forms and ages at such spreading centres, which traditional models predict to be magma-starved and cold, remains poorly understood. CAYSEIS project was proposed to survey the Cayman Trough area in order to obtain new data that constraints the nature of the crust, tectonic structures, lithologies outcropping and hydrothermal processes taking place in this area, which includes the Mid Cayman ultra-slow spreading centre (MSCS) with spreading rates of ~15-17 mm/yr. Understanding the sub-seabed geophysical structure of the MCSC is key to understanding not only the lithologies and structures exposed at the seabed, but more fundamentally, how they are related at depth and what role hydrothermal fluid flow plays in the geodynamics of ultraslow spreading. CAYSEIS was a joint and multidisciplinary programme of German, British and US American top tier scientists designed for the obtaining of a new high-quality dataset, including 3D Wide-Angle Seismic (WAS), magnetic, gravimetric and seismological data. We took leverage of the CAYSEIS dataset to invert a 3D velocity model of the Cayman Trough lithosphere using the Tomo3D code (Meléndez et al., 2015; 2019). This is one of the first times that the Tomo3D code is used for 3D inversion of real datasets. Thus, we are checking our results comparing them with travel time tomographic inversions of 2D lines and testing the different parameters to obtain the more accurate and higher resolution model as possible. The results of this experiment show not only the lithospheric structure along and across the MSCS, including the exhumed Ocean Core Complexes in the surrounding areas, but the 3D lithospheric configuration of the region which is important to understand the crustal formation processes and evolution of ultra-slow spreading settings
DescriptionEuropean Geosciences Union (EGU) General Assembly, 19-30 Apr 2021.-- 1 page
Publisher version (URL)https://doi.org/10.5194/egusphere-egu21-1545
URIhttp://hdl.handle.net/10261/259414
DOI10.5194/egusphere-egu21-1545
Appears in Collections:(ICM) Comunicaciones congresos




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