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Etudes et évaluation de processus océaniques par des hiérarchies ...

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225<br />

Chapter 9<br />

Abyssal and Overturning Circulation<br />

tel-00545911, version 1 - 13 Dec 2010<br />

The study of the <strong>de</strong>ep circulation of the world ocean has historically relied on the analysis of<br />

water masses. The reasons are that: (i) in the <strong>de</strong>ep water masses change very slowly in time<br />

as they are not subject to boundary forcing and as they give an integrated view of the velocity<br />

field which mostly weakens when <strong>de</strong>scending into the <strong>de</strong>pth of the ocean; (ii) it is technically<br />

difficult to measure the mo<strong>de</strong>rate but highly variable velocities in the <strong>de</strong>ep ocean, especially<br />

from a ship that is transported by the stronger currents at the ocean surface.<br />

In 1751 Stephen Hales constructed a “buck<strong>et</strong> sea-gage” and asked Henry Ellis, the captain<br />

of the Earl of Halifax, to perform temperature measurements in the <strong>de</strong>ep North Atlantic. Ellis<br />

found that temperature <strong>de</strong>creases with <strong>de</strong>pth and noted: “This experiment, which seemed at<br />

first but mere food for curiosity, became in the interim very useful to us. By this means we<br />

supplied our cold bath, and cooled our wines or water at pleasure; which is vastly agreeable to<br />

us in this burning climate.”<br />

It was Count Rumford who noted in 1800 that this cold water can only originate from high<br />

latitu<strong>de</strong>s and called it “[...] an inconvertible proof of the existing of cold water at the bottom<br />

of the sea, s<strong>et</strong>ting from the poles towards the equator.” This picture was then refined and the<br />

zones of formation of the <strong>de</strong>ep waters were i<strong>de</strong>ntified to lie in the high latitu<strong>de</strong>s of the North<br />

Atlantic and the Antarctic Ocean. There is no formation of <strong>de</strong>ep waters in the Indian and<br />

Pacific Ocean. The <strong>de</strong>ep waters are upwelling in the rest of the ocean counter balancing the<br />

diffusion of heat into the <strong>de</strong>ep ocean and thus forming the thermocline , that is a more or less<br />

sharp boundary b<strong>et</strong>ween the warm surface waters and the cold <strong>de</strong>ep waters in the mid and low<br />

latitu<strong>de</strong>s. These processes are schematised in fig. 9.1.<br />

North Pole<br />

✻<br />

Z<br />

convection<br />

✛<br />

✛<br />

North Atlantic<br />

surface layer (warm)<br />

Equator<br />

thermocline<br />

✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻ ✻<br />

upwelling upwelling upwelling<br />

❄❄❄<br />

✲<br />

<strong>de</strong>ep layer (cold)<br />

✲<br />

Figure 9.1: Overturning Circulation<br />

51

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