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  • 11
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 289(2010), 3/4, Seite 323-333, 1385-013X
    In: volume:289
    In: year:2010
    In: number:3/4
    In: pages:323-333
    Description / Table of Contents: We report here the first detailed 2D tomographic image of the crust and upper mantle structure of a Cretaceous seamount that formed during the interaction of the Pacific plate and the Louisville hotspot. Results show that at not, vert, similar ~1.5 km beneath the seamount summit, the core of the volcanic edifice appears to be dominantly intrusive, with velocities faster than 6.5 km/s. The edifice overlies both high lower crustal (〉 7.2-7.6 km/s) and upper mantle (〉 8.3 km/s) velocities, suggesting that ultramafic rocks have been intruded as sills rather than underplated beneath the crust. The results suggest that the ratio between the volume of intra-crustal magmatic intrusion and extrusive volcanism is as high as not, vert, similar ~4.5. In addition, the inversion of Moho reflections shows that the Pacific oceanic crust has been flexed downward by up to not, vert, similar ~2.5 km beneath the seamount. The flexure can be explained by an elastic plate model in which the seamount emplaced upon oceanic lithosphere that was not, vert, similar ~10 Myr at the time of loading. Intra-crustal magmatic intrusion may be a feature of hotspot volcanism at young, hot, oceanic lithosphere, whereas, magmatic underplating below a pre-existing Moho may be more likely to occur where a hotspot interacts with oceanic lithosphere that is several tens of millions of years old.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 12
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 282(2009), 1/4, Seite 47-55, 1385-013X
    In: volume:282
    In: year:2009
    In: number:1/4
    In: pages:47-55
    Description / Table of Contents: Breakup of the North Atlantic during the early tertiary was accompanied by widespread and massive magmatism, resulting in the coverage of large areas of the North Atlantic with flood basalts. These flood basalts hamper seismic investigations of underlying sequences and thus the understanding of the rifting, subsidence and evolution of the margin which, in turn, increases the risk for hydrocarbon exploration. In this paper we present a methodology for the simultaneous joint inversion of diverse geophysical datasets, i.e. free air gravity and magnetotelluric soundings (MT) using seismic a priori constraints. The attraction of the joint inversion approach is that different geophysical measurements are sensitive to different properties of the sub-surface, so through joint inversion we significantly reduce the null space and produce a single model that fits all datasets within a predefined tolerance. Using sensitivity analysis of synthetic data, we show how each data set contains complementary important information of the supra and sub-basalt structure. While separate inversions of individual datasets fail to image through the basalt layer, our joint inversion approach leads to a much improved sub-basalt structure. Application of the joint inversion algorithm to satellite gravity data and MT data acquired on the FLARE10 seismic line south west of Faroe islands supports the existence of a 1 km to 2 km thick low velocity region that might be indicative of the existence of a sedimentary basin underneath the basalt layer. Though in this paper we demonstrate the use of joint inversion on a sub-basalt target, we believe it has wider applicability to other areas where conventional seismic imaging fails.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 13
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 311(2011), 3/4, Seite 275-286, 1385-013X
    In: volume:311
    In: year:2011
    In: number:3/4
    In: pages:275-286
    Description / Table of Contents: The genesis of oceanic crust at intermediate to fast spreading ridges occurs by the crystallization of mantle melts accumulated in at least one shallow melt lens situated below the ridge axis. Seismic reflection data suggest that the depth of this melt lens is inversely correlated with spreading rate and thereby magma supply. The heat released in it by crystallization and melt injection is removed by a combination of hydrothermal cooling and diffusion. Due to the different time scales of hydrothermal cooling and crustal accretion, numerical models have so far focused on only one of the two processes. Here we present the results from a coupled model that solves simultaneously for crustal accretion and hydrothermal cooling. Our approach resolves both processes within one 2D finite-element model that self-consistently solves for crustal, mantle, and hydrothermal flow. The formation of new oceanic crust is approximated as a gabbro glacier, in which the entire lower crust crystallizes in one shallow melt lens. We find that the depth of the melt lens and the shape of hot (potentially molten) lower crust are highly dependent on the ridge permeability structure. The predicted depth of the melt lens is primarily controlled by the permeability at the ridge axis, whereas the off-axis permeability determines the width of hot lower crust. A detailed comparison of the modeling results with observed locations of the melt lens at intermediate to fast spreading ridges shows that only a relatively narrow range of crustal permeabilities is consistent with observations. In addition, we find significant deviations between models that resolve or parameterize hydrothermal cooling: the predicted crustal thermal structures show major differences for models that predict the same melt lens location. This illustrates the importance of resolving hydrothermal flow in simulations of crustal accretion.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 14
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 260(2007), 3/4, Seite 505-515, 1385-013X
    In: volume:260
    In: year:2007
    In: number:3/4
    In: pages:505-515
    Type of Medium: Online Resource
    Pages: Ill., graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 15
    Online Resource
    Online Resource
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 272(2008), 1/2, Seite 422-428, 1385-013X
    In: volume:272
    In: year:2008
    In: number:1/2
    In: pages:422-428
    Description / Table of Contents: The Cape Verde Islands are located on a mid-plate topographic swell and are thought to have formed above a deep mantle plume. Wide-angle seismic data have been used to determine the crustal and uppermost mantle structure along a ~ 440 km long transect of the archipelago. Modelling shows that 'normal' oceanic crust, ~ 7 km in thickness, exists between the islands and is gently flexed due to volcano loading. There is no direct evidence for high density bodies in the lower crust or for an anomalously low density upper mantle. The observed flexure and free-air gravity anomaly can be explained by volcano loading of a plate with an effective elastic thickness of 30 km and a load and infill density of 2600 kg m- 3. The origin of the Cape Verde swell is poorly understood. An elastic thickness of 30 km is expected for the ~ 125 Ma old oceanic lithosphere beneath the islands, suggesting that the observed height of the swell and the elevated heat flow cannot be attributed to thermal reheating of the lithosphere. The lack of evidence for high densities and velocities in the lower crust and low densities and velocities in the upper mantle, suggests that neither a crustal underplate or a depleted swell root are the cause of the shallower than expected bathymetry and that, instead, the swell is supported by dynamic uplift associated with the underlying plume.
    Type of Medium: Online Resource
    ISSN: 1385-013X
    Language: English
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  • 16
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 269(2008), 1/2, Seite 118-130, 1385-013X
    In: volume:269
    In: year:2008
    In: number:1/2
    In: pages:118-130
    Description / Table of Contents: Segmentation along convergent margins controls earthquake magnitude and location, but the physical causes of segment boundaries, and their impact on earthquake rupture dynamics, are still poorly understood. One aspect of the 2004 and 2005 great Sumatra-Andaman earthquakes is their abrupt termination along a common boundary. This has led to speculation on the nature of the boundary, its origin and why it was not breached. For the first time the boundary has been imaged and, with newly acquired marine geophysical data, we demonstrate that a ridge on the subducting Indo-Australian oceanic crust may exert a control on margin segmentation. This suggests a lower plate influence on margin structure, particularly its segmentation. The ridge is masked by the sedimentary cover in the trench. Its most likely trend is NNE-SSW. It is interpreted as a fracture zone on the subducting oceanic plate. A ramp or tear along the eastern flank of the subducting fracture zone beneath Simeulue Island may be considered as an intensification factor in terms of rupture propagation barrier.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 17
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 255(2007), 3/4, Seite 414-431, 1385-013X
    In: volume:255
    In: year:2007
    In: number:3/4
    In: pages:414-431
    Description / Table of Contents: High-resolution multi-frequency and multi-component seismic data were acquired at northern Hydrate Ridge in the accretionary complex of the Cascadia subduction zone to quantify the amount of hydrate and free gas in the sediment. We present a detailed local analysis of four component (4C) ocean bottom seismometer (OBS) data and show the importance of multi-frequency and shear wave data for determining hydrate reservoir properties. A detailed model of the elastic parameters at the bottom simulating reflector (BSR) is developed by using synthetic seismogram modelling. The main focus in this study is an amplitude-versus-offset (AVO) analysis of shear waves, which originate by PS-conversion at the BSR in 73 m below the seafloor (bsf). The AVO analysis enables the determination of the shear wave velocity above the BSR. A velocity of 400 m/s indicates that the presence of gas hydrate in the pore space significantly increases the shear modulus of the sediment above the BSR. Information about the attenuation and the shape of the BSR transition zone is obtained from the frequency-dependent reflection amplitudes of the BSR. The BSR is shown to be a gradual type transition zone of 1.5-2.5 m thickness. Average Q factors of Qp = 150 for P-waves and of Qs = 35 for S-waves are determined within the gas hydrate stability zone (GHSZ). The low Qs factor points to a pronounced attenuation of S-waves in the uppermost sediments. From rock physics modelling, the hydrate concentration is estimated to vary locally between 3-12% of the pore space. Below the BSR, free gas concentrations of 0.5% and 8% are determined for homogeneous and patchy distributed gas, respectively.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 18
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 275(2008), 1/2, Seite 61-69, 1385-013X
    In: volume:275
    In: year:2008
    In: number:1/2
    In: pages:61-69
    Description / Table of Contents: During segment-scale studies of the southern Mid-Atlantic Ridge (MAR), 712° S, we found evidence in the water column for high-temperature hydrothermal activity, off-axis, east of Ascension Island. Extensive water column and seafloor work using both standard CTD and deep submergence AUV and ROV deployments led to the discovery and sampling of the Drachenschlundʺ (Dragon Throatʺ) black smoker vent at 8ʿ17.87? S/13ʿ30.45? W in 2915 m water depth. The vent is flanked by several inactive chimney structures in a field we have named Nibelungenʺ. The site is located 6 km south of a non-transform offset between two adjacent 2nd-order ridge-segments and 9 km east of the presently-active, northward-propagating A2 ridge-segment, on a prominent outward-facing fault scarp. Both vent-fluid compositions and host-rock analyses show this site to be an ultramafic-hosted system, the first of its kind to be found on the southern MAR. The thermal output of this single vent, based on plume rise-height information, is estimated to be 60 ± 15 MW. This value is high for a single black smokerʺ vent but small for an entire field. The tectonic setting and low He content of the vent fluids imply that high-temperature off-axis venting at Drachenschlundʺ is driven not by magmatic processes, as at the majority of on-axis hydrothermal systems, but by residual heat minedʺ from the deeper lithosphere. Whether this heat is being extracted from high-temperature mantle peridotites or deep crustal cumulates formed at the duellingʺ non-transfrom offset is unclear, in either case the Drachenschlund vent provides the first direct observations of how cooling of deeper parts of the lithosphere, at least at slow-spreading ridges, may be occurring.
    Type of Medium: Online Resource
    Pages: Ill., grap. Darst
    ISSN: 1385-013X
    Language: English
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  • 19
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 270(2008), 3/4, Seite 338-348, 1385-013X
    In: volume:270
    In: year:2008
    In: number:3/4
    In: pages:338-348
    Type of Medium: Online Resource
    Pages: graph. Darst.
    ISSN: 1385-013X
    Language: English
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  • 20
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 277(2009), 3/4, Seite 514-524, 1385-013X
    In: volume:277
    In: year:2009
    In: number:3/4
    In: pages:514-524
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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