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

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4.6. ESTIMATION OF FRICTION PARAMETERS AND LAWS IN 1.5D SHALLOW-WATER GRAVI<br />

Ocean Dynamics<br />

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

when consi<strong>de</strong>ring the estimation of the <strong>par</strong>am<strong>et</strong>er values<br />

(see below).<br />

5.2 Discriminating b<strong>et</strong>ween laws<br />

In the previous subsection, we <strong>de</strong>monstrated that the<br />

assimilation procedure manages to estimate the right<br />

<strong>par</strong>am<strong>et</strong>er values in the case of linear and quadratic<br />

friction. The type of the friction law was, however,<br />

imposed before the estimation procedure, a feature that<br />

we relax now. That is, we still use the same data but<br />

the assimilation procedure does not know with which<br />

kind of friction law the data were produced and what<br />

the corresponding <strong>par</strong>am<strong>et</strong>er value is. We investigate<br />

in experiments G00001 and G00010 if the assimilation<br />

scheme obtains the <strong>par</strong>am<strong>et</strong>er values and, in this way,<br />

manages to d<strong>et</strong>ermine the friction law. We emphasise<br />

that the difference to experiments A00001 and A00010<br />

is that, now, the assimilation scheme does not know<br />

that the other <strong>par</strong>am<strong>et</strong>er is vanishing, but it has to<br />

establish it.<br />

The results are presented in Fig 4. The initial ensemble<br />

of the <strong>par</strong>am<strong>et</strong>er values is the same for both<br />

experiments. In both cases, we see a good convergence<br />

to the right values and, thus, a clear d<strong>et</strong>ermination of<br />

the right friction law.<br />

5.3 Estimating both <strong>par</strong>am<strong>et</strong>ers<br />

The next step is to consi<strong>de</strong>r dynamics which inclu<strong>de</strong><br />

both friction laws. The procedure is i<strong>de</strong>ntical to that<br />

of the previous subsection, only that now, both <strong>par</strong>am<strong>et</strong>er<br />

values are non-vanishing. There are in<strong>de</strong>ed a<br />

large number of examples where the friction law passes<br />

from linear to quadratic and where both laws coexist<br />

(see Schlichting and Gertsen 2000 pp. chap 1.3). In<br />

cases where one friction law is established, the friction<br />

coefficient (weakly) <strong>de</strong>pends on the Reynolds number.<br />

By allowing for two, or more, friction laws, not only<br />

the optimal value of the friction <strong>par</strong>am<strong>et</strong>er is estimated<br />

but also its variation with the Reynolds number (see<br />

Section 6). The case of estimating both τ and c D at the<br />

same time is more challenging, as they both inclu<strong>de</strong><br />

friction in the mo<strong>de</strong>l dynamics and have, to the first<br />

or<strong>de</strong>r, the same effect on the gravity current, that is,<br />

make it move down-slope. Furthermore, we choose,<br />

in experiments G0021, G0121, and G0221, values for<br />

τ and c D such that they have a similar magnitu<strong>de</strong> of<br />

the friction force, that is τ ≈ c D |u| and |u| = √ u 2 + v 2 ,<br />

which is the most challenging case. A large number<br />

of experiments have been performed with different<br />

values of the friction <strong>par</strong>am<strong>et</strong>ers, the results show no<br />

qualitative differences. In Fig. 5, the convergences of<br />

the <strong>par</strong>am<strong>et</strong>er values are shown. In general, one notices<br />

a good convergence in τ-c D -space of all members of<br />

the ensemble towards the true values. A b<strong>et</strong>ter convergence<br />

for runs with lower perturbations σ (noise level)<br />

is noticed. A further reduction of the variance of the<br />

noise ad<strong>de</strong>d to the observations (necessary to make<br />

the EnKF consistent; see Burgers <strong>et</strong> al. 1998) leads to<br />

a divergence of the EnKF. A conspicuous feature of<br />

Fig. 5 is the fact that the ensemble is aligned along<br />

a straight line, which corresponds to a space-timemean<br />

absolute velocity of the gravity current of<br />

Fig. 4 Distribution of the ensemble in τ (horizontal direction)<br />

and c D (vertical direction) space for the two experiments: G0001<br />

(black dots) and G0011 (red dots), at different times: Initial distribution<br />

(left) (some initial values lie outsi<strong>de</strong> the area shown), after<br />

7 days (middle) and after seven iterations of the 7-day dynamics<br />

(right). The values of τ and c D are normalised by the true value<br />

used in the control run (see Table 1). The experiment shows a<br />

successful convergence towards the true values. The black dots<br />

converge to (τ, c D ) = (τ 0 , 0) and the red dots to (τ, c D ) = (0, c D0 )

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