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Titlebook: Oceanography of the Ross Sea Antarctica; Antarctica Giancarlo Spezie,Giuseppe M. R. Manzella Conference proceedings 1999 Springer-Verlag It

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Thermohaline Data and Ocean Circulation on the Ross Sea Continental Shelfoles. Using representative salinity and temperature transects from the summers of 1962-63, 1976-77 and 1983-84, we briefly review the ocean stratification and circulation, identifying five primary water masses. Year-round salinity.profiles at a single location in 1960-61 and early winter temperature
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Upper Ocean Thermal Structure and Fronts Between New Zealand and the Ross Sea (Austral Summer 1994–195 on the basis of four high resolution XBT sections, and during the summer 1995-96 with two high resolution XBT sections. The area of investigation is almost completely (with the exception of the southernmost part) interested by the Antarctic Circumpolar Current (ACC). The main fronts (SubAntarctic
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The Large-Scale Thermohaline Structure of the Ross Gyrecluding about 7,000 historical and modern hydrographic stations. A new regional climatology was obtained through the objective analysys of the data on neutral surfaces. Steric height anomaly maps portray Ross Gyre as a depression south of the mid-ocean ridge between about 170°E and 140°W. The centre
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Reconstructing the General Circulation of the Ross Sea (Antarctica) Using a Robust Diagnostic Model field, while temperature and salinity values have been objectively analyzed from data acquired during the Xth Italian expedition in Antarctic. Even if model assumptions could be improved (e.g. enhance the description of the sea-ice interaction, use available wind time series and updated topography)
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A Wind and Boundary Driven Circulation Model of the Ross Seaport as induced locally by the wind and forced by the external action of the East Wind Drift during the ice-free season. Furthermore, the implementation of the same model with higher resolution to a coastal area including Terra Nova Bay has provided information on the local circulation regime. The c
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Wintertime Expansion and Contraction of the Terra Nova Bay Polynyatuations in the Terra Nova Bay polynya. It has long been believed that the Terra Nova Bay polynya opens in response to strong offshore katabatic wind forcing. This study shows that not only is the sensible heat flux important in controlling fluctuations in polynya extent, but that the longwave heat
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