Frontal structure and Antarctic Bottom Water flow through the Princess Elizabeth Trough, Antarctica (original) (raw)

1999, Deep Sea Research Part I: Oceanographic Research Papers

Hydrographic, current meter and ADCP data collected during two recent cruises in the South Indian Ocean (RRS Discovery cruise 200 in February 1993 and RRS Discovery cruise 207 in February 1994) are used to investigate the current structure within the Princess Elizabeth Trough (PET), near the Antarctic continent at 853E, 63}663S. This gap in topography between the Kerguelen Plateau and the Antarctic continent, with sill depth 3750 m, provides a route for the exchange of Antarctic Bottom Water between the Australian}Antarctic Basin and the Weddell}Enderby Basin. Shears derived from ADCP and hydrographic data are used to deduce the barotropic component of the velocity "eld, and thus the volume transports of the water masses. Both the Southern Antarctic Circumpolar Current Front (SACCF) and the Southern Boundary of the Antarctic Circumpolar Current (SB) pass through the northern PET (latitudes 63 to 64.53S) associated with eastward transports. These are deep-reaching fronts with associated bottom velocities of several cm s\. Antarctic Bottom water (AABW) from the Wed-dell}Enderby Basin is transported eastwards in the jets associated with these fronts. The transport of water with potential temperatures less than 03C is 3 ($1) Sv. The SB is shown to meander in the PET, caused by the cyclonic gyre immediately west of the PET in Prydz Bay. The AABW therefore also meanders before continuing eastwards. In the southern PET (latitudes 64.5 to 663S) a bottom intensi"ed #ow of AABW is observed #owing west. This AABW has most likely formed not far from the PET, along the Antarctic continental shelf and slope to the east. Current meters show that speeds in this #ow have an annual scalar mean of 10 cm s\. The transport of water with potential temperatures less than 03C is 20 ($3) Sv. The southern PET features westward #ow throughout the water column, since the shallower depths 0967-0637/99/$ } see front matter 1999 Elsevier Science Ltd. All rights reserved. PII: S 0 9 6 7 -0 6 3 7 ( 9 8 ) 0 0 0 1 0 8 -3 #ow of bottom water, the total westward transport of the whole water column in the southern PET is 45 ( $6) Sv.

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Formation and circulation of the water masses between the southern Indian Ocean and Antarctica: Results from δ18O

Journal of Marine Research, 1999

We present measurements of the stable isotopes of oxygen ( 18 O and 16 O) from seawater samples collected during the Antarctic Deep Out ow Experiment (ADOX) cruises in the Southern Ocean and southern Indian Ocean, February to . The data are used in conjunction with hydrographic data to infer characteristics of the formation and circulation of water masses found in the region. The waters on the continental shelf of Antarctica (adjacent to the Princess Elizabeth Trough; PET) are isotopically the lightest found due to the injection of about 1% of glacial meltwater, and are probably advected to the region from farther east by the current associated with the Antarctic Slope Front. They appear to be locally disassociated from the Antarctic Surface Water and Winter Water (WW) farther north in the PET. The WW of the Enderby Basin is isotopically lighter than the PET WW and also fresher, indicating the presence of an additional component of glacial meltwater or high-latitude precipitation. North of the Antarctic Circumpolar Current, the surface d 18 O values correlate strongly with salinity, but extrapolate to an apparent freshwater endmember which is isotopically too light to be reasonable; advection and mixing of the water masses dominate over the local water balance at this location.

The baroclinic transport of the Antarctic Circumpolar Current south of Africa

Geophysical Research Letters, 2005

Five hydrographic transects at nominal longitudes 0°E and 30°E, and fourteen expendable bathythermograph (XBT) sections near the former longitude are used to study the baroclinic transport of the Antarctic Circumpolar Current (ACC) between Africa and Antarctica. The bottom-referenced geostrophic transport between the Subtropical Front and the ACC Southern Boundary is 147±10 Sv. Estimating the transport from the XBTs using a technique previously employed south of Australia proves delicate because of an irregular bathymetry and water mass variations. It nevertheless confirms ACC transports around 150 Sv. Gathering these and other estimates from the Atlantic sector suggests that, while North Atlantic Deep Water is injected in the current west of 35°W, a partially compensating loss of Deep Circumpolar Water occurs east of this longitude. Another transport increase from 0°E to 30°E might reflect southward transfer across the Subtropical Front south of the Agulhas retroflection.

Circulation and transport of water masses in the Lazarev Sea, Antarctica, during summer and winter 2006

Deep Sea Research Part I: Oceanographic Research Papers, 2011

The distribution and circulation of water masses in the region between 61W and 31E and between the Antarctic continental shelf and 601S are analyzed using hydrographic and shipboard acoustic Doppler current profiler (ADCP) data taken during austral summer 2005/2006 and austral winter 2006. In both seasons two gateways are apparent where Warm Deep Water (WDW) and other water masses enter the Weddell Gyre through the Lazarev Sea: (a) a probably topographically trapped westward, then southwestward circulation around the northwestern edge of Maud Rise with maximum velocities of about 20 cm s À 1 and (b) the Antarctic Coastal Current (AntCC), which is confined to the Antarctic continental shelf slope and is associated with maximum velocities of about 25 cm s À 1 .

Shallow water modeling of Antarctic Bottom Water crossing the equator

Journal of Geophysical Research, 2004

1] The dynamics of abyssal equator-crossing flows are examined by studying simplified models of the flow in the equatorial region in the context of reduced-gravity shallow water theory. A simple ''frictional geostrophic'' model for one-layer cross-equatorial flow is described, in which geostrophy is replaced at the equator by frictional flow down the pressure gradient. This model is compared via numerical simulations to the one-layer reduced-gravity shallow water model for flow over realistic equatorial Atlantic Ocean bottom topography. It is argued that nonlinear advection is important at key locations where it permits the current to flow against a pressure gradient, a mechanism absent in the frictional geostrophic model and one of the reasons this model predicts less cross-equatorial flow than the shallow water model under similar conditions. Simulations of the shallow water model with an annually varying mass source reproduce the correct amplitude of observed time variability of cross-equatorial flow. The time evolution of volume transport across specific locations suggests that mass is stored in an equatorial basin, which can reduce the amplitude of time dependence of fluid actually proceeding into the Northern Hemisphere as compared to the amount entering the equatorial basin. Observed time series of temperature data at the equator are shown to be consistent with this hypothesis.

Antarctic bottom and lower circumpolar deep water circulation in the eastern Indian Ocean

Journal of Geophysical Research, 2006

Net northward transport below g n > 28.1 kg m À3 (%3200 m) into the Perth Basin of between 4.4 and 5.8 Sv is estimated from a year-long current meter mooring array between the Broken and Naturaliste plateaus. Northward transport of between 2.0 and 2.5 Sv of Antarctic Bottom Water (g n > 28.2 kg m À3), that must upwell within the southern region of the Perth Basin, results in an area-averaged diapycnal velocity and diffusivity of w* = 2.5-3.1 Â 10 À6 m s À1 and k = 13-15 Â 10 À4 m 2 s À1 , respectively. Diffusivity estimates for the Perth Basin are several times larger than area-averaged mixing estimates for the abyssal subtropical South Atlantic and Pacific oceans. However, the dissipation of turbulent kinetic energy required to maintain the abyssal mixing in the Perth Basin, = O(10 À9 W kg À1), is similar to that required in the South Atlantic Ocean. The areaaveraged diffusivity in the Perth Basin does not require unreasonable energy dissipation rates as this ocean basin is only weakly stratified. The abyssal diffusivity of the Perth Basin results from intense mixing at the basin boundary and in the basin interior over rough topography. The complex bathymetry and low abyssal stratification suggests that the Indian Ocean, for a given energy dissipation, may support a larger meridional overturning circulation than other subtropical basins.

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