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60<br />

80<br />

100<br />

−45<br />

−50<br />

−55<br />

Pressure (dbar)<br />

120<br />

140<br />

160<br />

180<br />

−60<br />

−65<br />

−70<br />

−75<br />

200<br />

220<br />

−80<br />

−85<br />

19.6 19.7 19.8 19.9 20 20.1 20.2 20.3 20.4<br />

Longitude ( o )<br />

−90<br />

60<br />

80<br />

100<br />

−45<br />

−50<br />

−55<br />

Pressure (dbar)<br />

120<br />

140<br />

160<br />

180<br />

−60<br />

−65<br />

−70<br />

−75<br />

200<br />

220<br />

−80<br />

−85<br />

19.6 19.7 19.8 19.9 20 20.1 20.2 20.3 20.4<br />

Longitude ( o )<br />

−90<br />

Figure 3.6: Transect as in Fig. 3.5, but for Turner angles in the diusive convective regime, with Tu<br />

< −48.81 ◦ (dark red) or R ρ > 1/15 as the lower bound of diusive convection.<br />

2.5 nm that any patterns smaller than about 9 km can be biased methodically.<br />

Presented observations from the M-8 eld campaign however show that the detected mesoscale<br />

patterns are vertically coherent over larger spatial scales. These phenomena probably result<br />

from dierent processes acting on dierent spatiotemporal scales. It may be speculated that<br />

intrusions, which have been initially coherent over larger spatial scales were, at this late-stage<br />

of the inow, already distorted by the strain eld of mesoscale motions. The σ θ contours in<br />

Fig. 3.5 b suggest that there were a few eddies in and below the halocline during M-8. For<br />

33

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