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J. Phys. , 9(3): 531554. Mantyla, A. W. and J. L. Reid (1983). Abyssal characteristics of the World Ocean waters. Deep Sea Res. 30(8A): 805-833. Martinson, D. , 1991. Open ocean convection in the Southern Ocean. This Volume. Martinson, D. G, 1990. Evolution of the Southem Ocean winter mixed layer and sea-ice: open ocean deepwater formation and ventilation. Jour. Geop. Res. 95(C7): 11,641-11,654 - 35 Martinson, D. , P. D. Killworth, and A. L. Gordon, 1981. A convective model for the Weddell Polynya.
1983). , 1990) and related modeling work (Martinson, 1990) have allowed a more detailed understanding of the processes controlling open Ocean deep convection. In particular, these reveal the following. , 1989). Lateral property gradients are essentially negligible within the regimes except in the vicinity of the front separating them and near Maud Rise where topographic influences are significant (Gordon and Huber, 1990). , 1989). 4OC in the cold regime. In both regimes this represents a strong source of heat isolated from the surface by a very thin and weak pycnocline - the Brunt-Vaisalafrequency across the pycnocline is typical of values in the deep Ocean elsewhere (Gordon, 1981).
39 In the austral summer of 1977, immediately following the last large polynya occurrence, Gordon (1978) observed a deep chimney at -67' S, 8' W (Figure 1). This cold, fresh, nearly homogeneous feature, overlain by a summer surface layer (-190 m thick), extended to -3000 m depth and had a radius (-13 km) that was comparable to the Rossby radius of deformation (-1 1 km). Gordon (1978) speculated that the feature was one, of many, remnant convective cells associated with the polynya which had been present in the area two months earlier.