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  • 1
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 2018
    In:  Journal of Geophysical Research: Oceans Vol. 123, No. 10 ( 2018-10), p. 7382-7392
    In: Journal of Geophysical Research: Oceans, American Geophysical Union (AGU), Vol. 123, No. 10 ( 2018-10), p. 7382-7392
    Kurzfassung: The single abyssal water source for the Panama Basin is the flow through the Ecuador Trench Critical flow theory suggests an abyssal water inflow of 0.29 ± 0.07 Sv The effect of geothermal heating can reach as high as 2,200‐m depth or 500 m above the abyssal water layer
    Materialart: Online-Ressource
    ISSN: 2169-9275 , 2169-9291
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 2018
    ZDB Id: 2016804-4
    ZDB Id: 161667-5
    ZDB Id: 3094219-6
    SSG: 16,13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 2018
    In:  Journal of Geophysical Research: Oceans Vol. 123, No. 10 ( 2018-10), p. 7393-7406
    In: Journal of Geophysical Research: Oceans, American Geophysical Union (AGU), Vol. 123, No. 10 ( 2018-10), p. 7393-7406
    Kurzfassung: Geothermal heating is the strongest water mass transformation process for abyssal waters inside the Panama Basin Almost all abyssal water mass transformations occur within the weakly stratified bottom boundary layer (wsBBL) hundreds of meters thick The thickness of the wsBBL may be used to differentiate the basin walls form the basin bottom
    Materialart: Online-Ressource
    ISSN: 2169-9275 , 2169-9291
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 2018
    ZDB Id: 2016804-4
    ZDB Id: 161667-5
    ZDB Id: 3094219-6
    SSG: 16,13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 3
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 2018
    In:  Journal of Geophysical Research: Oceans Vol. 123, No. 8 ( 2018-08), p. 5587-5598
    In: Journal of Geophysical Research: Oceans, American Geophysical Union (AGU), Vol. 123, No. 8 ( 2018-08), p. 5587-5598
    Kurzfassung: Properties of the weakly stratified bottom boundary layer (wsBBL) are mapped The density γ wsBBL and pressure P wsBBL at the upper boundary of the wsBBL are highly correlated The γ wsBBL – P wsBBL relation is used to differentiate global ocean subbasins and locations of intensive water transformation
    Materialart: Online-Ressource
    ISSN: 2169-9275 , 2169-9291
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 2018
    ZDB Id: 2016804-4
    ZDB Id: 161667-5
    ZDB Id: 3094219-6
    SSG: 16,13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 4
    In: Biogeosciences, Copernicus GmbH, Vol. 12, No. 2 ( 2015-01-27), p. 489-512
    Kurzfassung: Abstract. Ocean observations are analysed in the framework of Collaborative Research Center 754 (SFB 754) "Climate-Biogeochemistry Interactions in the Tropical Ocean" to study (1) the structure of tropical oxygen minimum zones (OMZs), (2) the processes that contribute to the oxygen budget, and (3) long-term changes in the oxygen distribution. The OMZ of the eastern tropical North Atlantic (ETNA), located between the well-ventilated subtropical gyre and the equatorial oxygen maximum, is composed of a deep OMZ at about 400 m in depth with its core region centred at about 20° W, 10° N and a shallow OMZ at about 100 m in depth, with the lowest oxygen concentrations in proximity to the coastal upwelling region off Mauritania and Senegal. The oxygen budget of the deep OMZ is given by oxygen consumption mainly balanced by the oxygen supply due to meridional eddy fluxes (about 60%) and vertical mixing (about 20%, locally up to 30%). Advection by zonal jets is crucial for the establishment of the equatorial oxygen maximum. In the latitude range of the deep OMZ, it dominates the oxygen supply in the upper 300 to 400 m and generates the intermediate oxygen maximum between deep and shallow OMZs. Water mass ages from transient tracers indicate substantially older water masses in the core of the deep OMZ (about 120–180 years) compared to regions north and south of it. The deoxygenation of the ETNA OMZ during recent decades suggests a substantial imbalance in the oxygen budget: about 10% of the oxygen consumption during that period was not balanced by ventilation. Long-term oxygen observations show variability on interannual, decadal and multidecadal timescales that can partly be attributed to circulation changes. In comparison to the ETNA OMZ, the eastern tropical South Pacific OMZ shows a similar structure, including an equatorial oxygen maximum driven by zonal advection but overall much lower oxygen concentrations approaching zero in extended regions. As the shape of the OMZs is set by ocean circulation, the widespread misrepresentation of the intermediate circulation in ocean circulation models substantially contributes to their oxygen bias, which might have significant impacts on predictions of future oxygen levels.
    Materialart: Online-Ressource
    ISSN: 1726-4189
    Sprache: Englisch
    Verlag: Copernicus GmbH
    Publikationsdatum: 2015
    ZDB Id: 2158181-2
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 5
    In: Earth and Planetary Science Letters, Elsevier BV, Vol. 531 ( 2020-02), p. 115991-
    Materialart: Online-Ressource
    ISSN: 0012-821X
    RVK:
    Sprache: Englisch
    Verlag: Elsevier BV
    Publikationsdatum: 2020
    ZDB Id: 300203-2
    ZDB Id: 1466659-5
    SSG: 16,13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 6
    Online-Ressource
    Online-Ressource
    Copernicus GmbH ; 2013
    In:  Biogeosciences Vol. 10, No. 7 ( 2013-07-26), p. 5079-5093
    In: Biogeosciences, Copernicus GmbH, Vol. 10, No. 7 ( 2013-07-26), p. 5079-5093
    Kurzfassung: Abstract. The replenishment of consumed oxygen in the open ocean oxygen minimum zone (OMZ) off northwest Africa is accomplished by oxygen transport across and along density surfaces, i.e. diapycnal and isopycnal oxygen supply. Here the diapycnal oxygen supply is investigated using a large observational set of oxygen profiles and diapycnal mixing data from years 2008 to 2010. Diapycnal mixing is inferred from different sources: (i) a large-scale tracer release experiment, (ii) microstructure profiles, and (iii) shipboard acoustic current measurements plus density profiles. From these measurements, the average diapycnal diffusivity in the studied depth interval from 150 to 500 m is estimated to be 1 × 10−5 m2 s−1, with lower and upper 95% confidence limits of 0.8 × 10−5 m2 s−1 and 1.4 × 10−5 m2 s−1. Diapycnal diffusivity in this depth range is predominantly caused by turbulence, and shows no significant vertical gradient. Diapycnal mixing is found to contribute substantially to the oxygen supply of the OMZ. Within the OMZ core, 1.5 μmol kg−1 yr−1 of oxygen is supplied via diapycnal mixing, contributing about one-third of the total demand. This oxygen which is supplied via diapycnal mixing originates from oxygen that has been laterally supplied within the upper Central Water layer above the OMZ, and within the Antarctic Intermediate Water layer below the OMZ. Due to the existence of a separate shallow oxygen minimum at about 100 m depth throughout most of the study area, there is no net vertical oxygen flux from the surface layer into the Central Water layer. Thus all oxygen supply of the OMZ is associated with remote pathways.
    Materialart: Online-Ressource
    ISSN: 1726-4189
    Sprache: Englisch
    Verlag: Copernicus GmbH
    Publikationsdatum: 2013
    ZDB Id: 2158181-2
    Standort Signatur Einschränkungen Verfügbarkeit
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