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

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46 CHAPITRE 4. ETUDES DE PROCESSUS OCÉANOGRAPHIQUES<br />

A. Wirth <strong>et</strong> al. / Deep-Sea Research II 49 (2002) 1279–1295 1283<br />

Fig. 3. Altim<strong>et</strong>ric sea-surface height anomalies (in mm) in early August for the years 1993, 1995, and 1996.<br />

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

downloa<strong>de</strong>d from: ftp.cls.fr/pub/oceano/AVISO/<br />

MSLA; d<strong>et</strong>ails can be found in Le Traon <strong>et</strong> al.<br />

(1998) and Le Traon and Ogor (1998). During the<br />

months of July and August, the GW could be<br />

d<strong>et</strong>ected by a sea-surface height anomaly (SSHA)<br />

which is maximum in the regions b<strong>et</strong>ween 61N and<br />

121N and b<strong>et</strong>ween 501E and 561E: As seen from<br />

Fig. 3, the location of the GW maximum is usually<br />

located within this area. Each SSHA map was also<br />

inspected visually. At later times of the GW<br />

evolution, that is, in September and October, the<br />

i<strong>de</strong>ntification of the GW was ambiguous as it<br />

som<strong>et</strong>imes splits up, was dominated by a stronger<br />

Socotra gyre (see Fig. 1), or had left the region<br />

<strong>de</strong>scribed above. We therefore have restricted our<br />

analysis of the GW position to the months of July<br />

and August.<br />

3. The mo<strong>de</strong>ls<br />

When analyzing ocean dynamics with the use of<br />

complex numerical mo<strong>de</strong>ls, a balance b<strong>et</strong>ween<br />

realism, comprehension and feasibility has to be<br />

found. To this end, it is often useful to employ a<br />

hierarchy of mo<strong>de</strong>ls of different complexities, to<br />

untangle the ocean dynamics. We therefore have<br />

employed two different classes of mo<strong>de</strong>ls, namely<br />

a fully thermodynamic multi-level primitive<br />

equation (PE) mo<strong>de</strong>l and a reduced-gravity (RG)<br />

mo<strong>de</strong>l.<br />

The rationale for this choice is as follows. The<br />

PE mo<strong>de</strong>l permits a fairly realistic simulation of<br />

the circulation, however, at a high computational<br />

expense so that only very few integrations were<br />

possible. The RG mo<strong>de</strong>l is much simpler and lags<br />

many important processes that are represented in<br />

the PE mo<strong>de</strong>l such as, for example, baroclinic<br />

instability, the influence of salinity and realistic<br />

topography. This has important effects on the<br />

solution, as mentioned in Section 5. However, a<br />

large number of experiments with a higher<br />

horizontal resolution are possible with the RG<br />

mo<strong>de</strong>l that can help to evaluate the chaotic nature<br />

of the ocean circulation.<br />

Each mo<strong>de</strong>l has been used in two configurations,<br />

with high and low friction, in or<strong>de</strong>r to<br />

estimate the sensitivity of the solution to the<br />

dissipation <strong>par</strong>am<strong>et</strong>rization.<br />

3.1. Primitive equation mo<strong>de</strong>l<br />

The PE mo<strong>de</strong>l was constructed on the basis of<br />

the MOM2.1 co<strong>de</strong> with a 1=31 1=31 resolution<br />

and 35 vertical levels, 10 of which are in the upper<br />

110 m: The mo<strong>de</strong>l extends from 301S to 261N and<br />

from 301E to 1101E; with open boundaries at 301S<br />

and at 1151E (Indonesian Throughflow) that are

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