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1
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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Associated Volumes
  • 2
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 269(2008), 1/2, Seite 41-55, 1385-013X
    In: volume:269
    In: year:2008
    In: number:1/2
    In: pages:41-55
    In: extent:15
    Description / Table of Contents: We examine the micro-earthquake seismicity recorded by two temporary arrays of ocean bottom seismometers on the outer rise offshore southern Chile on young oceanic plate of ages 14 Ma and 6 Ma, respectively. The arrays were in operation from December 2004January 2005 and consisted of 17 instruments and 12 instruments, respectively. Approximately 10 locatable events per day were recorded by each of the arrays. The catalogue, which is complete for magnitudes above 1.21.5, is characterized by a high b value, i.e., a high ratio of small to large events, and the data set is remarkable in that a large proportion of the events form clusters whose members show a high degree of waveform similarity. The largest cluster thus identified consisted of 27 similar events (average inter-event correlation coefficient N0.8 for a 9.5 s window), and waveform similarity persists far into the coda. Inter-event spacing is irregular, but very short waiting times of a few minutes are far more common than expected from a Poisson distribution. Seismicity with these features (high b value, large number of similar events with short waiting times) is typical of swarm activity, which, based on empirical evidence and theoretical considerations, is generally thought to be driven by fluid pressure variations. Because no pronounced outer rise bulge exists on the very young plate in the study region, it is unlikely that melt is accessible from decompression melting or opening of cracks. A fluid source related to processes at the nearby ridge is conceivable for the younger segment but less likely for the older one. We infer that the fluid source could be seawater, which enters through fractures in the crust. Most of the similarearthquake clusters are within the crust, but some of them locate significantly below the Moho. If our interpretation is correct, this implies that water is present within the mantle. Hydration of the mantle is also indicated by a decrease of Pn velocities below the outer rise seen on a refraction profile through one of the arrays [Contreras-Reyes, E., Grevemeyer, I., Flueh, E.R., Scherwath, M., Heesemann, M., 2007. Alteration of the subducting oceanic lithosphere at the southern central Chile trench-outer rise. Geochem., Geophys. Geosyst. 8, Q07003.]. The deepest events within the array on the 6 Ma old plate occur where the temperature reaches 500600 ʿC, consistent with the value observed for large intraplate earthquakes within the mantle (650 ʿC), suggesting that the maximum temperature at which these fluid-mediated micro-earthquakes can occur is similar or identical to that of large earthquakes.
    Type of Medium: Online Resource
    Pages: 15 , graph. Darst., Kt
    ISSN: 1385-013X
    Language: English
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  • 3
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 269(2008), 3/4, Seite 570-575, 1385-013X
    In: volume:269
    In: year:2008
    In: number:3/4
    In: pages:570-575
    Type of Medium: Online Resource
    ISSN: 1385-013X
    Language: English
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  • 4
    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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  • 5
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 273(2008), 1/2, Seite 175-183, 1385-013X
    In: volume:273
    In: year:2008
    In: number:1/2
    In: pages:175-183
    Description / Table of Contents: Three ferromanganese crusts from the northeast, northwest and central Atlantic were re-dated using osmium (Os) isotope stratigraphy and yield ages from middle Miocene to the present. The three Os isotope records do not show evidence for growth hiatuses. The reconstructed Os isotope-based growth rates for the sections older than 10 Ma are higher than those determined previously by the combined beryllium isotope (10Be/9Be) and cobalt (Co) constant-flux methods, which results in a decrease in the maximum age of each crust. This re-dating does not lead to significant changes to the interpretation of previously determined radiogenic isotope neodymium, lead (Nd, Pb) time series because the variability of these isotopes was very small in the records of the three crusts prior to 10 Ma. The Os isotope record of the central Atlantic crust shows a pronounced minimum during the middle Miocene between 15 and 12 Ma, similar to a minimum previously observed in two ferromanganese crusts from the central Pacific. For the other two Atlantic crusts, the Os isotope records and their calibration to the global seawater curve for the middle Miocene are either more uncertain or too short and thus do not allow for a reliable identification of an isotopic minimum. Similar to pronounced minima reported previously for the Cretaceous/Tertiary and Eocene/Oligocene boundaries, possible interpretations for the newly identified middle Miocene Os isotope minimum include changes in weathering intensity and/or a meteorite impact coinciding with the formation of the Nördlinger Ries Crater. It is suggested that the eruption and weathering of the Columbia River flood basalts provided a significant amount of the unradiogenic Os required to produce the middle Miocene minimum.
    Type of Medium: Online Resource
    Pages: graph. Darst
    ISSN: 1385-013X
    Language: English
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  • 6
    In: Earth and planetary science letters, Amsterdam [u.a.] : Elsevier, 1966, 273(2008), 3/4, Seite 260-269, 1385-013X
    In: volume:273
    In: year:2008
    In: number:3/4
    In: pages:260-269
    Type of Medium: Online Resource
    Pages: graph. Darst.
    ISSN: 1385-013X
    Language: English
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  • 7
    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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  • 8
    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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  • 9
    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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  • 10
    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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