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

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231<br />

Chapter 10<br />

Pen<strong>et</strong>ration of Surface Fluxes<br />

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

The ocean is mostly driven by the fluxes of heat, fresh water and momentum at its surface.<br />

The influence of these fluxes are, however, not only felt in a thin layer at the ocean surface, but<br />

influence the dynamics of the entire ocean. In this chapter we discuss how the forcing applied<br />

at the surface of the ocean pen<strong>et</strong>rates into the <strong>de</strong>pth of the ocean.<br />

For the processes of vertical pen<strong>et</strong>ration, it is clear that we can no longer neglect the<br />

dynamics in the vertical direction, and the shallow water equations are not adapted for the<br />

processes studied here (with the exception of gravity currents). We thus have to look for other<br />

simplifications of the the full three-dimensional Navier-Stokes equations. A first guess might<br />

be to neglect the dynamics all tog<strong>et</strong>her and pr<strong>et</strong>end that the transport to the interior is due<br />

to molecular motions, that is viscosity and diffusivities (for heat and salt). This possibility is<br />

discussed and refuted in section 10.1.<br />

In section 10.2 we show, using the Navier-Stokes equations and some “hand-waving” that<br />

the three dimensional dynamics at small scales creates some viscous and diffusive behavior at<br />

large scales. This i<strong>de</strong>a is the basis of all realistic calculations not only in ocean dynamics but<br />

in fluid dynamics in general.<br />

10.1 Molecular Transport<br />

The molecular thermal diffusivity of sea water is κ ≈ 10 −7 m 2 s −1 . The diffusion equation in the<br />

vertical is given by,<br />

∂ t T = ∂ z (κ∂ z T). (10.1)<br />

We further suppose that there is a periodic heat flux of magnitu<strong>de</strong> Q at the surface (boundary<br />

condition), that is:<br />

∂ z T | z=0 = Q cos(2πt/τ + π/4). (10.2)<br />

c p ρκ<br />

The linear equation (10.1) with the boundary conditions (10.2) has the solution:<br />

with:<br />

T(z,t) = T A e −z/L cos(2πt/τ − z/L), (10.3)<br />

T A = Q √ √ τ τκ<br />

c p ρ 2πκ and L = π . (10.4)<br />

57

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