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  • Ocean temperature  (10)
  • Chemistry
  • Inorganic Chemistry
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  • Massachusetts Institute of Technology and Woods Hole Oceanographic Institution  (11)
  • 2010-2014  (11)
  • 1
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution March 1988
    Description: Inverse methods are applied to historical hydrographic data to address two aspects of the general circulation of the Atlantic Ocean. The method allows conservation statements for mass and other properties, along with a variety of other constraints, to be combined in a dynamically consistent way to estimate the absolute velocity field and associated property transports. The method is first used to examine the exchange of mass and heat between the South Atlantic and the neighboring ocean basins. The Antarctic Circumpolar Current (ACC) carries a surplus of intermediate water into the South Atlantic through Drake Passage which is compensated by a surplus of deep and bottom water leaving the basin south of Africa. As a result, the ACC loses .25±.18x1015 W of heat in crossing the Atlantic. At 32°S the meridional flux of heat is .25±.19x1015 W equatorward, consistent in sign but smaller in magnitude than other recent estimates. This heat flux is carried primarily by a meridional overturning cell in which the export of 17 Sv of North Atlantic Deep Water (NADW) is balanced by an equatorward return flow equally split between the surface layers, and the intermediate and bottom water. No "leak" of warm Indian Ocean thermocline water is necessary to account for the equatorward heat flux across 32°S; in fact, a large transfer of warm water from the Indian Ocean to the Atlantic is found to be inconsistent with the present data set. Together these results demonstrate that the Atlantic as a whole acts to convert intermediate water to deep and bottom water, and thus that the global thermohaline cell associated with the formation and export of NADW is closed primarily by a "cold water path," in which deep water leaving the Atlantic ultimately returns as intermediate water entering the basin through Drake Passage. The second problem addressed concerns the circulation and property fluxes across 24°and 36°N in the subtropical North Atlantic. Conservation statements are considered for the nutrients as well as mass, and the nutrients are found to contribute significant information independent of temperature and salinity. Silicate is particularly effective in reducing the indeterminacy of circulation estimates based on mass conservation alone. In turn, the results demonstrate that accurate estimates of the chemical fluxes depend on relatively detailed knowledge of the circulation. The zonal-integral of the circulation consists of an overturning cell at both latitudes, with a net export of 19 Sv of NADW. This cell results in a poleward heat flux of 1.3±.2x1015 Wand an equatorward oxygen flux of 2900±180 kmol S-l across each latitude. The net flux of silicate is also equatorward: 138±38 kmol s-1 and 152±56 kmol s -1 across 36°and 24° N, respectively. However, in contrast to heat and oxygen, the overturning cell is not the only important mechanism responsible for the net silicate transport. A horizontal recirculation consisting of northward flow of silica-rich deep water in the eastern basin balanced by southward flow of low silica water in the western basin results in a significant silicate flux to the north. The net equatorward flux is thus smaller than indicated by the overturning cell alone. The net flux of nitrate across 36°N is n9±35 kmol 8- 1 to the north and is indistinguishable from zero at 24°N (-8±39 kmol 8-1 ), leading to a net divergence of nitrate between these two latitudes. Forcing the system to conserve nitrate leads to an unreasonable circulation. The dominant contribution to the nitrate flux at 36°N results from the correlation of strong northward flow and relatively high nitrate concentrations in the sub-surface waters of the Gulf Stream. The observed nitrate divergence between 24°and 36°N, and convergence north of 36°N, can be accounted for by a shallow cell in which the northward flow of inorganic nitrogen (nitrate) in the Gulf Stream is balanced by a southward flux of dissolved organic nitrogen in the recirculation gyre. Oxidation of the dissolved organic matter during its transit of the subtropical gyre supplies the required source of regenerated nitrate to the Gulf Stream and consumes oxygen, consistent with recent observations of oxygen utilization in the Sargasso Sea.
    Description: This research was supported by NASA under contract NAG5-534 and NSF under contract OCE-8521685.
    Keywords: Ocean circulation ; Ocean temperature ; Conrad (Ship) Cruise ; Atlantis II (Ship : 1963-) Cruise AII109
    Repository Name: Woods Hole Open Access Server
    Type: Thesis
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  • 2
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution January 1977
    Description: Millimeter scale fluctuations in refractive index recorded with a freely sinking shadowgraph system are correlated with finestructure profiles of temperature, salinity and density and compared to models of ocean turbulence. Images with vertically aligned periodic structure, called bands, are identified as salt fingers, while others with chaotic structure are turbulent. Images are found on interfaces that are 1-10m thick and have gradients at least several times the mean. From 6 profiles in the Mediterranean Outflow region of the eastern North Atlantic between 1.0 and 1.9 km depth, 398 interfaces have been identified and a significant fraction (about 1/3) of these have detectable images. High contrast images, including bands, are most often found below warm, saline intrusions and within stepped structure where there is a regular sequence of homogeneous mixed layers separated by interfaces. As the interfacial salinity gradient increases in the sense that allows salt finger convection, the fraction of interfaces with images increases. The horizontal spacing of bands (~5 mm) is consistent with calculated salt finger diameter. The calculated and observed length of ocean salt fingers (10-20 cm) is a small fraction of the interface thickness. High levels of small scale variability in the shadowgraphs is reflected in high levels of variance in the finestructure band of the temperature spectra. The temperature gradient spectra have a slope of -1, indicative of turbulence affected by buoyancy forces, and there is a relative peak at a wavelength near the observed salt finger length. The high contrast images are found at interfaces within the enhanced mean salinity gradient below saline intrusions. For very strong salinity gradients there is a solitary interface with intense images, but for weaker mean gradients the convection takes the form of stepped structure. The steps may evolve from the solitary interface as the salinity gradient is run down by salt finger convection. This study identifies parts of the ocean where salt finger convection is prevalent and includes the first comprehensive description of salt fingers in the ocean. Existing models of salt fingers are evaluated in light of ocean observations, and models of ocean turbulence are compared to measurements.
    Description: Support from ONR contract N00014-66-C0241 NR. 083-004 is also acknowledged.
    Keywords: Ocean temperature ; Oceanic mixing ; Salinity ; Turbulence ; Atlantis II (Ship : 1963-) Cruise AII76
    Repository Name: Woods Hole Open Access Server
    Type: Thesis
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  • 3
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 2000
    Description: Estimation of the upper ocean heat budget from one year of observations at a moored array in the north central Arabian Sea shows a rough balance between the horizontal advection and time change in heat when the one-dimensional balance between the surface heat flux and oceanic heat content breaks down. The two major episodes of horizontal advection, during the early northeast (NE) and late southwest (SW) monsoon seasons, are both associated with the propagation of mesoscale eddies. During the NE monsoon, the heat fluxes within the mixed layer are not significantly different from zero, and the large heat flux comes from advected changes in the thermocline depth. During the SW monsoon a coastal filament exports recently upwelled water from the Omani coast to the site of the array, 600 km offshore. Altimetry shows mildly elevated levels of surface eddy kinetic energy along the Arabian coast during the SW monsoon, suggesting that such offshore transport may be an important component of the Arabian Sea heat budget. The sea surface temperature (SST) and mixed layer depth are observed to respond to high frequency (HF, diurnal to atmospheric synoptic time scales) variability in the surface heat flux and wind stress. The rectified effect of this HF forcing is investigated in a three-dimensional reduced gravity thermodynamic model of the Arabian Sea and Indian Ocean. Both the HF heat and wind forcing act locally to increase vertical mixing in the model, reducing the SST. Interactions between the local response to the surface forcing, Ekman divergences, and remotely propagated signals in the model can reverse this, generating greater SSTs under HF forcing, particularly at low latitudes. The annual mean SST, however, is lowered under HF forcing, changing the balance between the net surface heat flux (which is dependent on the SST) and the meridional heat flux in the model. A suite of experiments with one-dimensional upper ocean models with different representations of vertical mixing processes suggests that the rectified effect of the diurnal heating cycle is dependent on the model, and overstated in the formulation used in the three-dimensional model.
    Description: Funded by the Office of Naval Research (ONR), grant NOOO14-94-1-0161 and National Defense Science and Engineering Graduate Fellowship and by ONR grant NOOO14-99-1-0090.
    Keywords: Monsoons ; Ocean temperature ; Ocean-atmosphere interaction
    Repository Name: Woods Hole Open Access Server
    Type: Thesis
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  • 4
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1996
    Description: A convection experiment was done with a rotating rectangular tank as a model of oceanic meridional overturning circulation. Heat flux was fixed at one bottom end of the tank using an electrical heater. Temperature was fixed at the other end using a cooling plate. All other boundaries were insulated. The cross sections of temperature field were made at several locations. In equilibrium, the heat input to the fluid H was the same as the meridional heat flux (heat flux from the source to the sink), so it was possible to find a scaling law relating H to the temperature difference across the tank ΔT and rotation rate f. The experimental result suggests that the meridional heat transport in the experiment was mostly due to geostrophic flows with a minor correction caused by the bottom friction. If there was no friction, the scaling law from the experiment resembles the one verified in part in the numerical model by Bryan and Cox (1967). Flow visualization and temperature sections showed that there were meridional geostrophic currents that transported heat. When the typical values of the North Atlantic are introduced, the geostrophic scaling law predicts meridional heat flux comparable to that estimated in the North Atlantic when the vertical eddy diffusivity of heat is about 1cm2s-1. Naturally, this experiment is a only crude model of the oceanic convective circulation. We do not claim that the geostrophic scaling applies in detail to the oceans, however, it may have some important use in climate modeling. For example, almost all existing box models and two-dimensional numerical models of ocean circulation use a frictional scaling law for buoyancy transport. A box model with the geostrophic scaling law is shown to be more robust to a change in the boundary forcing so that it is less likely to have a thermohaline catastrophic transition under the present conditions. It is also shown that a restoring boundary condition for salinity introduces stability to a thermal mode circulation, unless the restoring time for salinity is several orders of magnitude larger than that for temperature.
    Description: This study has been funded by NSF grant number OCE92-01464 and Korean Government Overseas Scholarship Grant.
    Keywords: Heat ; Rotating masses of fluid ; Ocean circulation ; Ocean temperature ; Thermoclines
    Repository Name: Woods Hole Open Access Server
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  • 5
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution May 1998
    Description: Planktonic protozoan grazers have the potential to significantly affect the chemistry of particle-associated trace metals. This is due both to the importance of protists as consumers of bacterial-sized particles, and to the unique low-pH, enzyme-rich microenvironment of the grazer food vacuole. This thesis examines the role of protozoan grazers in the marine geochemistry of strongly hydrolyzed, particle-reactive trace metals, in particular Th and Fe. A series of tracer experiments was carried out in model systems in order to determine the effect of grazer-mediated transformations on the chemical speciation and partitioning of radioisotopes C9Fe, 234Th, 51Cr) associated with prey cells. Results indicate that protozoan grazers are equally able to mobilize intracellular and extracellular trace metals. In some cases, protozoan regeneration of trace metals appears to lead to the formation of metal-organic complexes. Protozoan grazing may generate colloidal material that can scavenge trace metals and, via aggregation, lead to an increase in the metal/organic carbon ratio of aggregated particles. Model system experiments were also conducted in order to determine the effect of grazers on mineral phases, specifically colloidal iron oxide (ferrihydrite). Several independent techniques were employed, including size fractionation ors9Fe-labeled colloids, competitive ligand exchange, and iron-limited diatoms as "probes" for bioavailable Fe. Experimental evidence strongly suggests that protozoan grazing can affect the surface chemistry and increase the dissolution rate of iron oxide phases through phagotrophic ingestion. In further work on protozoan-mediated dissolution of colloidal Fe oxides, a novel tracer technique was developed based on the synthesis of colloidal ferrihydrite impregnated with 133Ba as an inert tracer. This technique was shown to be a sensitive, quantitative indicator for the extent of ferrihydrite dissolution/alteration by a variety of mechanisms, including photochemical reduction and ligand-mediated dissolution. In field experiments using this technique, grazing by naturally occuring protistan assemblages was shown to significantly enhance the dissolution rate of colloidal ferrihydrite over that in non-grazing controls. Laboratory and field results indicate that, when integrated temporally over the entire euphotic zone, protozoan grazing may equal or exceed photoreduction as a pathway for the dissolution of iron oxides.
    Description: This work was financially supported by a Department of Defense ONR-NDSEG Graduate Fellowship, Office ofNaval Research AASERT Award (N00014-94-1-0711), and the National Science Foundation EGB Program (OCE-9523910).
    Keywords: Protozoa ; Water chemistry ; Trace elements in water ; Marine zooplankton ; Chemistry
    Repository Name: Woods Hole Open Access Server
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  • 6
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 2010
    Description: The variability in the DWBC, its connection to the forcing in the northern North Atlantic and interaction with the Gulf Stream were explored from a combination of remote sensing and in-situ measurements in the western North Atlantic. Using satellite altimetry and Sea Surface Temperature (SST) we found evidence of the relation between changes in the Gulf Stream path and the variability in the temperature and velocity fields in the Slope Water. This relation was such that southward shifts of the main axis of the Gulf Stream were preceded by cold temperature anomalies and intensification of the southwestward flow. The analysis of 5.5 years of moored CTD and horizontal velocity data in the DWBC at 69°W recorded during the period 2002-2008, showed that the variability along the DWBC is linked to changes in the dense water formation regions. The evolution of potential vorticity (PV) at the mooring site, characterized by a transition from deep to upper Labrador Sea Water (LSW), was similar to that observed in the Labrador Sea 6 to 9 years earlier, and imply spreading rates for the LSW that varied over time from 1.5 to 2.5cm/s. The time dependence of the spreading rates was in good agreement with changes in the strength of the DWBC at the mooring site. The evolution of the DWBC transport was explored in more detail from a 5-element moored array, also at 69°W. The results, for the period of 2004-2008, were consistent with the single mooring analysis. The variability measured from the array showed that upper, intermediate and deep water mass layers expand and contract at each other’s expense, leading to alternating positive and negative PV anomalies at the upper-LSW, deep-LSW and Overflow Water (OW). Larger DWBC transports were associated with enhanced presence of recently ventilated upper-LSW and OW, rather than deep-LSW. The relative contribution of the different water masses to the observed circulation was investigated by inverting individual PV anomalies isolated from the observations. We found that changes in the depth-integrated circulation were mostly driven by changes in the OW.
    Description: During the first two years, my time here was funded through a La Caixa Foundation fellowship as well as an MIT presidential fellowship. Financial support for my thesis work was provided by National Science Foundation grants OCE-0241354 and OCE-0726720. Support for traveling to meetings was also provided by the MIT Houghton Fund and the WHOI Academic Programs Office.
    Keywords: Ocean currents ; Ocean temperature ; Endeavor (Ship: 1976-) Cruise EN256 ; Endeavor (Ship: 1976-) Cruise EN257 ; 440 ; Knorr (Ship : 1970-) Cruise KN173-2 ; Oceanus (Ship : 1975-) Cruise OC269 ; Oceanus (Ship : 1975-) Cruise OC401 ; Oceanus (Ship : 1975-) Cruise OC411 ; Oceanus (Ship : 1975-) Cruise OC417 ; Oceanus (Ship : 1975-) Cruise OC421 ; Oceanus (Ship : 1975-) Cruise OC432 ; Oceanus (Ship : 1975-) Cruise OC436 ; Oceanus (Ship : 1975-) Cruise OC446
    Repository Name: Woods Hole Open Access Server
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  • 7
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution September 1988
    Description: The highly energetic Agulhas Retroflection region south of the African continent lies at the junction of the South Indian, South Atlantic, and Circumpolar Oceans. A new survey of the Agulhas Retroflection taken in March 1985, plus historical hydrographic data, allow its dynamical and water-mass characteristics, and its role in exchanging mass, tracers, and vorticity between the three oceans, to be extensively characterized. The 1985 survey is composed of three independent, synoptic elements: a grid of closely-spaced, full-water-depth hydrographic stations (the first entirely full-water-column survey in this area), including several transects of the Agulhas and Agulhas Return Currents; a continuous survey of the path of the currents (the first such survey in the Agulhas); and a contemporaneous and relatively cloud-free sea surface temperature image derived from satellite infrared measurements. Mass transport balances within the closed grid boxes of the 1985 hydrographic survey provide information about current transport, recirculation (transport in excess of estimated returning interior ocean transport), and the overall Retroflection transport pattern. The current transport values exceed by as much as a factor of 1.5 the maximum interior transport computed from observed wind-stress curl and linear theory. Agulhas Current transports ranged from 56 to 95 x 106 m s-l at four 1985 transects crossing the current. Agulhas Return Current transports at the two 1985 transects were 54 and 65 x 106 m s-l. These transports are computed relative to 2400 dbar, which lies below the deep oxygen minimum emanating from the South Indian Ocean, and above the North Atlantic Deep Water salinity maximum. The current retroflected in two distinct branches in 1985, with a cold ring and a partially isolated warm recirculation cell found between the two branches. The satellite-derived sea surface temperature (SST) image, in agreement with the in situ measurements, showed that the cold ring lacked a cold SST anomaly; that the subsurface current path, as represented by a survey of the 15 C isotherm and 200 dbar surface intersection, was closely followed by a sharp front in sea surface temperature; and that most of the Agulhas's surface warm core retroflected upstream of the second retroflection branch. Anticyclonic curvature vorticity at sharp turns in the subsurface current path was found to exceed the maximum allowed by gradient wind balance, indicating that at these locations time-dependence and cross-frontal flow are important. The current's density field is found to meet necessary conditions for baroclinic and barotropic instability. These instability mechanisms may play a role in ring formation and current meandering. Top-to-bottom cross-stream spatial and isopycnal water-mass layering in the Agulhas Current, Agulhas Return Current, and associated rings are presented in two sets of sections, one contoured with pressure and the other with potential density as vertical coordinate. Temperature, salinity, oxygen, potential density and velocity sections are shown contoured versus pressure; and pressure, salinity, oxygen, and planetary potential vorticity are shown contoured versus potential density. These sections clearly illustrate water-mass structure both in space and relative to isopycnal surfaces. Strong salt, oxygen, and potential vorticity fronts on isopycnals in the upper -300 m across the Agulhas and Agulhas Return Current are observed, as are deep western boundary filaments of (i) salty, low oxygen water at intermediate depths traceable to Red Sea Water influences, and (ii) salty North Atlantic Deep Water close round the tip of Africa. The 1985 cold-core ring is the first cold-cored isolated feature to be observed within the Retroflection itself. Its transport was 64 x 106 m s-1, its integrated kinetic and available potential energy anomalies were 8.3 and 61 x 1015 J respectively, and its integrated planetary potential vorticity anomaly was 2.8 x 10-12 m-1 s-1. The potential vorticity flux associated with the exchange of 25 warm ring/cold ring pairs per year between the South Indian and Southern Oceans would balance the potential vorticity input by the wind to the entire South Indian Ocean. Interbasin flow of warm thermocline water (warmer than 8 C) from the South Indian to the South Atlantic Ocean is reconsidered in light of the 1985 hydrographic data. Thermocline water flow from the South Indian Ocean into the South Atlantic in the 1985 and historical observations is found to range from 2.8 to 〈9.6 x 106 m s-I. These values are less than the S;10 x 106 m s·1 needed to balance the Atlantic Ocean export of deep water, and implies that the deep water export is balanced in part by water colder than 8 C.
    Description: Funding was provided by the Office of Naval Research under contract numbers NOOOI4-84-C-OI34 (NR083-400), NOOOI4-85-C-OOOl (NR083-004), and NOOOI4-87-K-0007 (NR083-004).
    Keywords: Ocean currents ; Ocean temperature ; Thomas Washington (Ship) Cruise 3 ; Knorr (Ship : 1970-) Cruise ; Oceanus (Ship : 1975-) Cruise
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  • 8
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution February 1993
    Description: The dynamical aspects involved in the assimilation of altimeter data in a numerical ocean model have been investigated. The model used for this study is a quasi-geostrophic model of the Gulf Stream region. The data that have been assimilated are maps of sea surface height which have been obtained as the superposition of sea surface height variability deduced from the Geosat altimeter measurements and a mean field constructed from historical hydrographic data. The method used for assimilating the data is the nudging technique. Nudging has been implemented in such a way as to achieve a high degree of convergence of the surface model fields toward the observations. We have analyzed the mechanisms of the model adjustment, and the final statistical equilibrium characteristics of the model simulation when the surface data are assimilated. Since the surface data are the superposition of a mean component and an eddy component, in order to understand the relative role of these two components in determining the characteristics of the final st atistical steady state, we have considered two different experiments: in the first experiment only the climatological mean field is assimilated, while in the second experiment the total surface streamfunction field (mean + eddies) has been used. We have found that the mean component of the surface data determines, to a large extent, the structure of the flow field in the subsurface layers, while the eddy field, as well as the inflow/outflow conditions at the open boundaries, affect its intensity. In particular, if surface eddies are not assimilated only a weak flow develops in the two deeper model layers where no inflow/ outflow is prescribed at the boundaries. Comparisons of the assimilation results with available in situ observations show a considerable improvement in the degree of realism of the climatological model behavior, with respect to the model in which no data are assimilated. In particular, the possibility of building into the model more realistic eddy characteristics, through the assimilation of the surface eddy field, proves very successful in driving components of the mean model circulation that are in good agreement with the available observations.
    Description: This research was carried out with the support of the National Aeronaut ics Space Administration, through a contract to MIT from the Jet Propulsion Laboratory, # 958208, as a part of the TOPEX-Poseidon investigation.
    Keywords: Ocean-atmosphere interaction ; Ocean currents ; Ocean temperature
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  • 9
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-25
    Description: Submitted in partial fulfillment of the requirements for the degree of Master of Science at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution May 1996
    Description: The relationship of planktonic foraminiferal populations and stable isotopes to synoptic sea surface temperatures (SST's) was examined in the Sea of Okhotsk, using sediment trap samples (trap deployed Aug. '90 - Aug. '91; 53°19'N, 149°50'E) and AVHRR satellite sea surface temperature data. Synoptic SST's for the deployment ranged between -1.2 and 14.8°C. Two species dominated total yearly foraminiferal flux: N. pachyderma (left) and G. bulloides, with 57% and 31% of yearly flux, respectively. Calcification depths (from δ180eq. calcite) for these species ranged between 20 and 40 meters. Due to the highly stratified water column in the Sea of Okhotsk, these foraminifera experienced temperatures much colder than SST, and use of standard paleotemperature proxies significantly underestimates SST. The average paleotemperatures calculated from both δ180pachy and δ18Dbull were 5-6°C lower than average synoptic SST. Faunal indicators were consistent with this finding, with the N. pachyderma left-to-right coiling ratios 〉98% for the entire trap deployment. These ratios would suggest maximum seasonal SST's no greater than 10°C, nearly 5°C colder than the actual sea surface temperature maximum. The results from this study indicate that in highly stratified water columns, standard paleotemperature proxies may yield results as much as 5°C cooler than actual sea surface conditions.
    Keywords: Marine plankton ; Ocean temperature
    Repository Name: Woods Hole Open Access Server
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  • 10
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    Massachusetts Institute of Technology and Woods Hole Oceanographic Institution
    Publication Date: 2022-05-26
    Description: Submitted in partial fulfillment of the requirements for the degree of Master of Science at the Massachusetts Institute of Technology and the Woods Hole Oceanographic Institution July 1991
    Description: Six hydrographic basinwide sections, two in each of the three major ocean basins, are employed in a set of inverse calculations to determine the extent of exchange between the Pacific and Indian Oceans through the Indonesian Archipelago and the net global oceanic heat flux at 30°S. Using a model which combines the data for the South Pacific and South Indian Oceans, it is found that even the largest existing estimates of Indonesian Passage through flow (20 Sv) are consistent with the data. However, the available information cannot limit the extent of the exchange, i.e. both smaller and larger through flows produce physically reasonable circulation patterns. The seasonal and interannual variations which have been found by other investigators and which we are incapable of resolving, lead us to conclude that in the long term mean an estimate of ~10 Sv for the through flow is most reasonable. Globally, at 30°S, we find a net oceanic heat flux of -1.1 ± 1.7 PW, which is not significantly different from zero. It is dominated by a large (〉1 PW) southward heat flux in the Indian Ocean. Large equatorward (~0.8 PW) heat flux values in the South Atlantic Basin are not consistent with our data. We therefore conclude that although our data are consistent with some water following the warm water return path for NADW (Gordon 1986), the cold water path must play the dominant role in the maintenance of the global thermohaline cell associated with the formation process of NADW.
    Keywords: Ocean temperature ; Ocean circulation
    Repository Name: Woods Hole Open Access Server
    Type: Thesis
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