Abstract
Abstract Oxygen, nutrient, and tritium concentrations observed in the western Labrador Sea in March 1976 during deep convective renewal of Labrador Sea water are analyzed to show how a newly formed water mass obtains its characteristics. Common to other winter observations of deep mixed layers, the oxygen concentrations are some 6% undersaturated, even in the upper 20 m. A gas transfer model coupled to a simple mixed layer model illustrates the difficulty of transferring sufficient oxygen across the air-sea boundary to fully oxygenate the mixed layer when the mixed layer depth exceeds a few hundred meters. The nutrient concentrations of the mixed layers are fairly well mixed as is consistent with the fairly narrow range of nutrient concentrations of the source waters. Only the tritium concentrations exhibit any structure within the mixed layer, and it is argued that this is due to the much larger range of tritium concentrations in the source waters that make up the mixed layer.
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