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  • 1
    Electronic Resource
    Electronic Resource
    Evolution of magma-poor continental margins from rifting to seafloor spreading (2001)
    [s.l.] : Macmillian Magazines Ltd.
    Nature 413 (2001), S. 150-154 
    Details
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] The rifting of continents involves faulting (tectonism) and magmatism, which reflect the strain-rate and temperature dependent processes of solid–state deformation and decompression melting within the Earth. Most models of this rifting have treated tectonism and magmatism separately, and ...
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1038/35093085
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  • 2
    Electronic Resource
    Electronic Resource
    Thin Crust On the Flanks of the Slow-Spreading Southwest Indian Ridge (1996)
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 125 (1996), S. 0 
    Details
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The Southwest Indian Ridge marks an end-member of mid-ocean ridge spreading rates, with a current full rate of only 13–15 mm a−1. Most thermal models of mid-ocean ridges suggest a decrease in crustal thickness at such slow spreading rates, because conductive heat loss from the upwelling asthenospheric mantle decreases the volume of melt generated by decompression. Seismic measurements of the thickness of crust formed at very slow-spreading ridges are sparse. We have reanalysed data from a two-ship, split spread seismic refraction experiment conducted in 1962 on the southern flank of the Southwest Indian Ridge (Francis & Raitt 1967). We used synthetic seismograms to model amplitude variations, which were carefully recorded by the original investigators. 1- and 2-D modelling suggests that the seismic velocity increases smoothly with depth within the igneous crust, with an unusually high velocity of ∼6.0 km s−1 near the top of the crust, increasing to ∼7.0 km s−1 just above the Moho, and a crustal thickness of 5 km. Converted shear waves yield a Poisson's ratio of 0.30±0.01 in the crust, which is intermediate between values for gabbros and serpentinized upper mantle. the crustal thickness is consistent with a passive mantle upwelling model of melt generation at mid-ocean ridges. the unusual velocity structure may indicate the presence of gabbroic rocks near the seabed, unroofed by extension.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1365-246X.1996.tb06541.x
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  • 3
    Electronic Resource
    Electronic Resource
    Poisson's ratio of a seaward-dipping reflector series, Hatton Bank (1993)
    Oxford, UK : Blackwell Publishing Ltd
    Geophysical journal international 115 (1993), S. 0 
    Details
    ISSN: 1365-246X
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: Seismic reflection profiles across the Hatton Bank continental margin in the eastern North Atlantic have imaged thick sequences of seaward-dipping reflectors. Converted shear waves propagating through one of these sequences were recorded on a two-ship expanding spread profile just landward of the ocean-continent transition. Synthetic seismogram modelling of these shear waves indicates that Poisson's ratio in the sequence is 0.27 ± 0.01, similar to that of normal oceanic Layer 2.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1111/j.1365-246X.1993.tb05608.x
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  • 4
    Electronic Resource
    Electronic Resource
    Internal deformation and compaction of the Makran accretionary wedge (1997)
    Oxford, UK : Blackwell Science Ltd
    Terra nova 9 (1997), S. 0 
    Details
    ISSN: 1365-3121
    Source: Blackwell Publishing Journal Backfiles 1879-2005
    Topics: Geosciences
    Notes: The Makran accretionary wedge is one of the largest on Earth. A 7-km-thick column of sands and quartzolithic turbidites are incorporated into this wedge in a series of deformed thrust sheets. We present the results of prestack depth migration and focusing-error analysis (migration velocity analysis) performed on a profile across the Makran wedge. The depth section shows the deformation style of the accreted sediments, and the migration velocities allow us to estimate porosity variations in the sediments. The thrust sheets show evidence of fault-propagation folding, with a long wavelength of deformation (≈ 12 km) and secondary thrusting in the kink bands of the folds, such that the central part of each thrust sheet is elevated to form an additional ridge. This deformation style and the 15° steep surface slope of the first ridge suggest a high degree of consolidation. Porosities were calculated from the seismic migration velocities and the ratio of fluid pressure to lithostatic pressure λ was estimated for 5 locations along the profile. Rather than being undercompacted and overpressured as in most accretionary wedges, the sedimentary input is normally compacted (exponential porosity decay) throughout almost the whole wedge. However, a slight increase in porosity and λ at depth, with respect to the normal compaction curve indicates, that the turbiditic sequence might be overpressured landward of the deformation front.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1046/j.1365-3121.1997.d01-13.x
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  • 5
    Electronic Resource
    Electronic Resource
    Accurate Modelling of Sonobuoy Refraction Data to Determine Velocity Variations in Oceanic Crust (1997)
    Springer
    Marine geophysical researches 19 (1997), S. 25-36 
    Details
    ISSN: 1573-0581
    Keywords: Seismic refraction ; sonobuoys ; modelling ; crustal structure
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract Modern disposable sonobuoys can provide a simple and cost-effective alternative to ocean bottom seismometers for marine refraction experiments over oceanic crust. Unfortunately, the fact that they are free to drift with the prevailing ocean currents can introduce significant travel-time errors into the modelling process if the seafloor topography is large. For sonobuoys recorded during and after turns the drift rate and direction can be uniquely determined by inversion of the shot-receiver ranges derived from the water-wave arrival. The same method can be used to determine a best fitting average drift vector for the whole dataset. A modification to conventional two-dimensional travel-time modelling techniques has been developed to account for this drift. Each sonobuoy profile is divided into several subsets, typically of 100 shots each, and each subset is then modelled as a separate common receiver gather, significantly reducing the errors in the calculated travel-times. For re alistic bathymetry, the magnitude of these travel-time errors is up to 200 ms, significantly larger than the estimated picking uncertainty. Real data from a typical sonobuoy refraction experiment on the Mid-Atlantic Ridge were modelled with and without the drift correction applied. Much of the lateral variation in the velocity structure was removed when the drift correction was applied, indicating that this structure was due to variations in the travel-times caused by sonobuoy drift.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1023/A:1004249108479
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  • 6
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    Compressional structures on the West Iberia rifted margin: controls on their distribution (2008)
    In:  Geological Society Special Publication 306: 169-183.
    Details
    Publication Date: 2008-10-08
    Description: The West Iberia margin is a magma-poor rifted margin that resulted from Jurassic to Cretaceous polyphase rifting leading to the opening of the North Atlantic Ocean. The Mesozoic rift structures were overprinted by two compressive tectonic events during Eocene and Miocene times resulting from collision between Iberia, Europe and Africa. The effects of these compressive tectonic events are expressed by faults and folds within the post-rift sedimentary sequence. We mapped and studied these Cenozoic deformation structures throughout the Southern Iberia Abyssal Plain (40{degrees}-41{degrees}N, 11{degrees}-13{degrees}W) on the basis of an extensive dataset of time migrated seismic profiles acquired by various academic institutions. Acoustic basement has also been analysed on the basis of its seismic aspect, in order to test potential relationships with the distribution of the post-rift sedimentary deformation. Our observations lead to three major conclusions concerning the deformation affecting the post-rift sediments in the Southern Iberia Abyssal Plain: (1) the deformation occurs within the zone of exhumed continental mantle and not at its transition to continental or oceanic crust; (2) it is localized within a zone overlying basement with well-defined seismic characteristics; and (3) it is closely related to the major topographic features observed in the ocean-continent transition. The localization of the deformation within the zone of exhumed continental mantle and not at its boundaries to the adjacent oceanic and continental crust suggests that the limits between the different types of crust are transitional rather than sharp. Our results show that the zone of exhumed continental mantle represents the weakest zone within the margin that is preferentially deformed during initial convergence. At higher convergence rates, this zone may coincide with the location of a future subduction.
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  • 7
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    The pore-scale distribution of sediment-hosted hydrates: evidence from effective medium modelling of laboratory and borehole seismic data (2009)
    In:  Geological Society Special Publication 319: 93-101.
    Details
    Publication Date: 2009-07-27
    Description: Much of our knowledge on hydrate distribution in the subsurface comes from interpretations of remote seismic measurements. A key step in such interpretations is an effective medium theory that relates the seismic properties of a given sediment to its hydrate content. A variety of such theories have been developed; these theories generally give similar results if the same assumptions are made about the extent to which hydrate contributes to the load-bearing sediment frame. We have further developed and modified one such theory, the self-consistent approximation/differential effective medium approach, to incorporate additional empirical parameters describing the extent to which both the sediment matrix material (clay or quartz) and the hydrate are load-bearing. We find that a single choice of these parameters allows us to match well both P and S wave velocity measurements from both laboratory and in situ datasets, and that the inferred proportion of hydrate that is load-bearing varies approximately linearly with hydrate saturation. This proportion appears to decrease with increasing hydrate saturation for gas-rich laboratory environments, but increases with hydrate saturation when hydrate is formed from solution and for an in situ example.
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  • 8
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    Observations from the Alpine Tethys and Iberia Newfoundland margins pertinent to the interpretation of continental breakup (2007)
    In:  Geological Society Special Publication 282: 291-324.
    Details
    Publication Date: 2007-12-18
    Description: Although the IberiaNewfoundland and Alpine Tethys margins are of different age and ultimately had a different fate, they share remarkable similarities. Both pairs of margins show a change from initially distributed and decoupled extension to later localized, coupled and asymmetric extension that results in thinning of the crust and exhumation of subcontinental mantle. The change in the mode of extension together with the localization of deformation reflects an evolution of the bulk rheology of the extending lithosphere. In this paper we summarize the pertinent geological observations for the IberiaNewfoundland and Alpine Tethys margins. We describe the stratigraphic evolution, the fault geometry, basin architecture, and magmatic and metamophic evolution of the two pairs of margins from initial rifting to final continental breakup. This description forms a basis for understanding the evolution of the bulk rheology and how the various processes interact during progressive lithospheric extension. For the IberiaNewfoundland and Alpine Tethys margins initial rifting appears to be controlled by inherited heterogeneities and mechanical localization processes, whereas final rifting and lithospheric rupture is controlled by serpentinization, magmatic and thermal weakening. At other margins, these modes may interact in a different way depending on the prerift conditions and the evolution of the rheology during rifting.
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  • 9
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    Controlled-source electromagnetic and seismic delineation of subseafloor fluid flow structures in a gas hydrate province, offshore Norway (2016)
    Oxford University Press
    Details
    Publication Date: 2016-06-23
    Description: Deep sea pockmarks underlain by chimney-like or pipe structures that contain methane hydrate are abundant along the Norwegian continental margin. In such hydrate provinces the interaction between hydrate formation and fluid flow has significance for benthic ecosystems and possibly climate change. The Nyegga region, situated on the western Norwegian continental slope, is characterized by an extensive pockmark field known to accommodate substantial methane gas hydrate deposits. The aim of this study is to detect and delineate both the gas hydrate and free gas reservoirs at one of Nyegga's pockmarks. In 2012, a marine controlled-source electromagnetic (CSEM) survey was performed at a pockmark in this region, where high-resolution 3-D seismic data were previously collected in 2006. 2-D CSEM inversions were computed using the data acquired by ocean bottom electrical field receivers. Our results, derived from unconstrained and seismically constrained CSEM inversions, suggest the presence of two distinctive resistivity anomalies beneath the pockmark: a shallow vertical anomaly at the underlying pipe structure, likely due to gas hydrate accumulation, and a laterally extensive anomaly attributed to a free gas zone below the base of the gas hydrate stability zone. This work contributes to a robust characterization of gas hydrate deposits within subseafloor fluid flow pipe structures.
    Keywords: Marine Geosciences and Applied Geophysics
    Print ISSN: 0956-540X
    Electronic ISSN: 1365-246X
    Topics: Geosciences
    Published by Oxford University Press on behalf of The Deutsche Geophysikalische Gesellschaft (DGG) and the Royal Astronomical Society (RAS).
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  • 10
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    Crustal structure of the Murray Ridge, northwest Indian Ocean, from wide-angle seismic data (2015)
    Oxford University Press
    Details
    Publication Date: 2015-05-10
    Description: The Murray Ridge/Dalrymple Trough system forms the boundary between the Indian and Arabian plates in the northern Arabian Sea. Geodetic constraints from the surrounding continents suggest that this plate boundary is undergoing oblique extension at a rate of a few millimetres per year. We present wide-angle seismic data that constrains the composition of the Ridge and of adjacent lithosphere beneath the Indus Fan. We infer that Murray Ridge, like the adjacent Dalrymple Trough, is underlain by continental crust, while a thin crustal section beneath the Indus Fan represents thinned continental crust or exhumed serpentinized mantle that forms part of a magma-poor rifted margin. Changes in crustal structure across the Murray Ridge and Dalrymple Trough can explain short-wavelength gravity anomalies, but a long-wavelength anomaly must be attributed to deeper density contrasts that may result from a large age contrast across the plate boundary. The origin of this fragment of continental crust remains enigmatic, but the presence of basement fabrics to the south that are roughly parallel to Murray Ridge suggests that it separated from the India/Seychelles/Madagascar block by extension during early breakup of Gondwana.
    Keywords: Marine Geosciences and Applied Geophysics
    Print ISSN: 0956-540X
    Electronic ISSN: 1365-246X
    Topics: Geosciences
    Published by Oxford University Press on behalf of The Deutsche Geophysikalische Gesellschaft (DGG) and the Royal Astronomical Society (RAS).
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