Temperature fluctuations and current shear in Antarctic Bottom Water at the Vema Sill

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Abstract

The Vema Channel acts as a major conduit for the equatorward spreading of Antarctic Bottom Water between the Argentine and Brazil Basins. For almost two years the thermal stratification above its saddle depth (4660 m) – called Vema Sill – was recorded by moored thermistors and current meters. The lowest 490 m of the water column was instrumented to monitor the well-developed benthic boundary layer of Antarctic Bottom Water. The latter can be subdivided into Weddell Sea Deep Water on the sea bed and lower Circumpolar Deep Water above it. The data show fluctuations on various scales including periods, each about 1–2 weeks long, when the abyssal stratification virtually disappeared. Assuming a stable ratio between density and temperature, time series of bulk Richardson numbers are estimated from temperature and current shear data. The results suggest a potential for intermittent episodes of locally generated vertical mixing.

Section snippets

Motivation and observational strategy

The intricate spreading of Antarctic Bottom Water, a fundamental component of the global thermohaline circulation, is strongly controlled by the ocean’s bathymetry. The Rio Grande Rise acts as a major topographic obstacle for the equatorward bottom water flow on the western side of the South Atlantic (Fig. 1). A restricted exchange of abyssal waters between the Argentine and the Brazil Basins is accomplished by deep flow through the Vema Channel. Its narrowest spot, known as Vema Sill, is only

Instrument performance and calibration

Here, we discuss the data handling of the five recording instruments looking upward from the near-bottom position. Their overall performance was quite satisfactory. The CTD recorder (V389105 in Table 2) was brand new. Because of a short-dated delivery we had to trust the manufacturer’s calibration from early 1998. The recorder was mounted on the rope in a vertical position. Technically the moored CTD instrument performed excellently. Short-term salinity fluctuations of O(0.02) occur in the

Temperature distribution across the sill

Prior to deployment of mooring V389, a short CTD section (Fig. 2) across the sill was occupied. Due to lack of ship time efforts were concentrated on the eastern side of the Vema Channel (for detail see cruise report, Schulz et al., 1999). Similar sections from previous occupations are published in the literature (i.e. Hogg et al., 1982, Speer and Zenk, 1993, Jungclaus and Vanicek, 1999). Three characteristics of the thermal stratification are noted which are typical for deep passages in the

Discussion

By having a closer look at the isotherm diagram (Fig. 5) we detect in the gradient region (above ∼4330 m) a series of stratification collapses. If we take fluctuations of the 0 °C-isotherm as an indicator of advected temperature signals, we count O(10) abrupt displacements. They are not at all restricted to warm Circumpolar Deep Water (CDW) layers but could also be triggered by a near-bottom signal of penetrating cold Weddell Sea Deep Water (WSDW). Such episodic changes can reach almost

Acknowledgements

This note on temperature fluctuations of Antarctic Bottom Water is dedicated to Matthias Tomczak, respected author of topic contributions to oceanic fronts and mixing. Both METEOR cruises were funded by the Deutsche Forschungsgemeinschaft, Bonn. Additional support came from the Bundesministerium für Bildung und Forschung, Berlin (03F0377B). Many thanks go to the captains and crews of the two METEOR cruises as well as to the technical staff of the former IfM department of Marine Physics. The

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