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

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4.2. THE PARAMETRIZATION OF BAROCLINIC INSTABILITY IN A SIMPLE MODEL69<br />

580 Journal of Marine Research [58, 4<br />

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

Figure 4. Temporal energy spectrum of c 2 for k 5 2p · 11 in three experiments 1, 2 and 4 (from top<br />

to bottom) after a 35-point-wi<strong>de</strong> boxcar smother was applied. The peaks correspond to the time<br />

scale of about 200 days.<br />

The rst point, (i), saying that the effect of baroclinic instability on the baroclinic<br />

large-scale gradient is super diffusive seems to contradict intuition. The intuitive picture is<br />

in<strong>de</strong>ed that the dynamics at the (small) scale of the baroclinicallymost unstable mo<strong>de</strong> has a<br />

diffusive effect on the large-scale gradient. The point, however, is that energy injected in<br />

the barotropic mo<strong>de</strong> does not stay at such small scales but casca<strong>de</strong>s to the large scales, as<br />

explained by the two-dimensional inverse energy casca<strong>de</strong> (Kraichnan, 1967). The effect of<br />

this barotropic large-scale dynamics, caused by baroclinic instability, on the baroclinic<br />

large-scale gradient has to be <strong>par</strong>am<strong>et</strong>erized as a super diffusive behavior. It is in<strong>de</strong>ed well<br />

known that a lack of scale se<strong>par</strong>ation b<strong>et</strong>ween the ‘‘large’’ scale and the <strong>par</strong>am<strong>et</strong>erized<br />

scales lead to super diffusive behavior (Avellaneda and Majda, 1992). The inverse casca<strong>de</strong><br />

is, however, halted by the b-effect at the Rhines scale; that is, the scale at which the<br />

meridional change of the Coriolis <strong>par</strong>am<strong>et</strong>er balances nonlinearity (see e.g., Rhines, 1975,<br />

and Held and Larichev, 1996). This indicates that a normal diffusive <strong>par</strong>am<strong>et</strong>erization<br />

might be adapted for scales much larger than the Rhines scale, that is for scales on the or<strong>de</strong>r<br />

of thousands of kilom<strong>et</strong>ers. Calculations of much higher resolution would be nee<strong>de</strong>d to<br />

d<strong>et</strong>ermine such behavior. This also shows that for the practical use of <strong>par</strong>am<strong>et</strong>erizing<br />

baroclinic instability in non-eddy-permitting ocean mo<strong>de</strong>ls and climate mo<strong>de</strong>ls, a super

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