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  • 1
    Publikationsdatum: 2022-05-26
    Beschreibung: Author Posting. © American Geophysical Union, 2008. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geochemistry Geophysics Geosystems 9 (2008): Q12005, doi:10.1029/2008GC002100.
    Beschreibung: The hot spot-influenced western Galápagos Spreading Center (GSC) has an axial topographic high that reaches heights of ∼700 m relative to seafloor depth ∼25 km from the axis. We investigate the cause of the unusual size of the axial high using a model that determines the flexural response to loads resulting from the thermal and magmatic structure of the lithosphere. The thermal structure simulated is appropriate for large amounts of cooling by hydrothermal circulation, which tends to minimize the amount of partial melt needed to explain the axial topography. Nonetheless, results reveal that the large axial high near 92°W requires that either the crust below the magma lens contains 〉35% partial melt or that 20% melt is present in the lower crust and at least 3% in the mantle within a narrow column (〈∼10 km wide) extending to depths of 45–65 km. Because melt fractions 〉35% in the crust are considered unreasonable, it is likely that much of the axial high region of the GSC is underlain by a narrow region of partially molten mantle of widths approaching those imaged seismically beneath the East Pacific Rise. A narrow zone of mantle upwelling and melting, driven largely by melt buoyancy, is a plausible explanation.
    Beschreibung: Ito was supported by grants NSF-OCE- 0327051 and NSF-OCE-0351234.
    Schlagwort(e): Axial high ; Galapagos Spreading Center ; Partial melt ; Lithospheric flexure
    Repository-Name: Woods Hole Open Access Server
    Materialart: Article
    Format: application/pdf
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  • 2
    Publikationsdatum: 2022-05-26
    Beschreibung: Author Posting. © American Geophysical Union, 2004. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Journal of Geophysical Research 109 (2004): B10310, doi:10.1029/2004JB003066.
    Beschreibung: Multichannel seismic reflection data are used to infer crustal accretion processes along the intermediate spreading Galapagos Spreading Center. East of 92.5°W, we image a magma lens beneath the ridge axis that is relatively shallow (1.0–2.5 km below the seafloor) and narrow (∼0.5–1.5 km, cross-axis width). We also image a thin seismic layer 2A (0.24–0.42 km) that thickens away from the ridge axis by as much as 150%. West of 92.7°W, the magma lens is deeper (2.5–4.5 km) and wider (0.7–2.4 km), and layer 2A is thicker (0.36–0.66 km) and thickens off axis by 〈40%. The positive correlation between layer 2A thickness and magma lens depth supports the interpretation of layer 2A as the extrusive volcanic layer with thickness controlled by the pressure on the magma lens and its ability to push magma to the surface. Our findings also suggest that narrower magma lenses focus diking close the ridge axis such that lava flowing away from the ridge axis will blanket older flows and thicken the extrusive crust off axis. Flow of lava away from the ridge axis is probably promoted by the slope of the axial bathymetric high, which is largest east of 92.5°W. West of ∼94°W the “transitional” axial morphology lacks a prominent bathymetric high and layer 2A no longer thickens off axis. We detect no magma lens west of 94.7°W where a small axial valley appears. The above changes can be linked to the westward decrease in the magma and heat flux associated with the fading influence of the Galapagos hot spot on the Galapagos Spreading Center.
    Beschreibung: This project was funded by NSF-OCE- 0002189.
    Schlagwort(e): Layer 2A ; Mid-ocean ridges ; Shallow melt lens
    Repository-Name: Woods Hole Open Access Server
    Materialart: Article
    Format: application/pdf
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  • 3
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    American Geophysical Union
    Publikationsdatum: 2022-10-26
    Beschreibung: Author Posting. © American Geophysical Union, 2019. This article is posted here by permission of American Geophysical Union for personal use, not for redistribution. The definitive version was published in Geophysical Research Letters 46(5), (2019):2704-2714, doi:10.1029/2019GL081919.
    Beschreibung: Seismic images and glider sections of the Gulf Stream front along the U.S. eastern seaboard capture deep, lens‐shaped submesoscale features. These features have radii of 5–20 km, thicknesses of 150–300 m, and are located at depths greater than 500 m. These are typical signatures of anticyclonic submesoscale coherent vortices. A submesoscale‐resolving realistic simulation, which reproduces submesoscale coherent vortices with the same characteristics, is used to analyze their generation mechanism. Submesoscale coherent vortices are primarily generated where the Gulf Stream meets the Charleston Bump, a deep topographic feature, due to the frictional effects and intense mixing in the wake of the topography. These submesoscale coherent vortices can transport waters from the Charleston Bump's thick bottom mixed layer over long distances and spread them within the subtropical gyre. Their net effect on heat and salt distribution remains to be quantified.
    Beschreibung: J. G. gratefully acknowledges support from the French government, managed by the French National Agency for Research (ANR), through programs ISblue (ANR‐17‐EURE‐0015) and LabexMER (ANR‐10‐LABX‐19) and from LEFE/IMAGO through the project AO2017‐994457‐RADII. Simulations were performed using HPC resources from GENCI‐TGCC (grant 2017‐A0010107638). Simulations output is available upon request. Seismic data were processed using the Echos software package by Paradigm, Matlab, and Generic Mapping Tools. The Eastern North America Margin Community Seismic Experiment was funded by the National Science Foundation under grant OCE‐1347498 and UNOLS; cruise data are freely available via the Marine Geoscience Data System Academic Seismic Portal at Lamont‐Doherty Earth Observatory (http://www.marine-geo.org/portals/seismic/). Spray glider observations in the Gulf Stream are available from http://spraydata.ucsd.edu and should be cited using the following DOI (10.21238/S8SPRAY2675; Todd & Owens, 2016). Spray glider operations were funded by the National Science Foundation (OCE‐1633911) and the Office of Naval Research (N000141713040).
    Beschreibung: 2019-08-27
    Schlagwort(e): Submesoscale coherent vortices ; Glider ; Seismic observations ; Gulf Stream ; Topographic interactions ; Charleston Bump
    Repository-Name: Woods Hole Open Access Server
    Materialart: Article
    Standort Signatur Einschränkungen Verfügbarkeit
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