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  • Elsevier  (3)
  • Hamburg : Leitstelle METEOR, Inst. für Meereskunde der Univ. Hamburg
  • 2005-2009  (3)
  • 2007  (3)
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  • 2005-2009  (3)
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  • 1
    Publication Date: 2019-09-23
    Description: We describe the deep structure of the south Colombian–northern Ecuador convergent margin using travel time inversion of wide-angle seismic data recently collected offshore. The margin appears segmented into three contrasting zones. In the North Zone, affected by four great subduction earthquakes during the 20th century, normal oceanic crust subducts beneath the oceanic Cretaceous substratum of the margin underlined by seismic velocities as high as 6.0–6.5 km/s. In the Central Zone the subducting oceanic crust is over-thickened beneath the Carnegie Ridge. A steeper slope and a well-developed, high velocity, Cretaceous oceanic basement characterizes the margin wedge. This area coincides with a gap in significant subduction earthquake activity. In the South Zone, the subducting oceanic crust is normal. The fore-arc is characterized by large sedimentary basins suggesting significant subsidence. Velocities in the margin wedge are significantly lower and denote a different nature or a higher degree of fracturing. Even if the distance between the three profiles exceeds 150 km, the structural segmentation obtained along the Ecuadorian margin correlates well with the distribution of seismic activity and the neotectonic zonation.
    Type: Article , PeerReviewed
    Format: text
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  • 2
    Publication Date: 2019-09-24
    Description: Water transported within the subducting oceanic lithosphere into the Earth's interior affects a wealth of subduction zone processes, including intraslab earthquakes and arc magmatism. In recent years growing evidence suggests that much of the hydration of oceanic plates occurs at the trench–ocean slope right before subduction. Here, normal faults are created while the rigid lithosphere bends into the trench. Offshore of Middle America, multi-channel seismic reflection imaging suggests that bending-related faults cut into the uppermost mantle, providing a mechanism for hydration and transformation of mantle peridotites into serpentinites. Seismic wide-angle reflection and refraction data were collected coincident with one of the seismic profiles where the faults have been imaged. Travel time inversion provides evidence that both crustal and uppermost mantle velocities are reduced with respect to the velocity structure found in mature oceanic crust away from deep-sea trenches. If mantle velocity reduction is solely produced by hydration, velocities indicate 10–15% of serpentinization in the uppermost 3 km of the mantle, where seismic data provide enough resolution. A small network of ocean bottom hydrophones, deployed for about a month, detected ∼ 3 local micro earthquakes per day. Earthquake epicentres align with fault scarps at the seafloor and continuous earthquake activity might be an important process to facilitate the percolation of seawater into the upper mantle.
    Type: Article , PeerReviewed
    Format: text
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  • 3
    Publication Date: 2018-07-19
    Description: Complete sediment subduction at the Costa Rica subduction zone makes this convergent margin an ideal place to investigate the effects of tectonic deformation in situ. We present a seismic reflection study along a line located 3 km landward of the Middle American Trench and oriented parallel to the strike of the décollement. The Ocean Bottom Hydrophone (OBH) seismic data include large offsets and incidence angles at the reflectors. We derive the P- and S-waves velocity distribution below the décollement using a P-wave analysis of amplitude with reflection angle. The investigation shows that there are unexpected large lateral velocity variations at a scale of only a few 100 m. The shear wave velocity in the uppermost subducted sediment varies between 300 and 700 m/s, while the variation of the compressional wave velocity is in a range of 1700 to 2000 m/s. The variation of the vP–vS ratio between 2.8 and 5.2 can only be explained by variations of the pore fluid pressure. The modelled velocities correspond to a normalised pore fluid pressure ratio λ* in the range between 0.02 and 0.93. The most reasonable explanation for these observations is the localised presence of fluids, which are released during diagenesis by smectite to illite transformation. During this process, which takes place in three discrete steps, the interlayer water of the smectite is added to the pore fluid and the permeability of the sediment is decreased. Both effects lead to the formation of small, overpressured cells.
    Type: Article , PeerReviewed
    Format: text
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