60
A. Simone et al.
ing and descending) were calculated at each cross-over point. Then, they were
interpolated linearly to common time (every 5 days) and used to dérivé the zonal
(u') and méridional (u') components of the geostrophic velocity fluctuations:
u ------ -——
2costp
V = ---- 2--- ±2sin(p
where

Vd are the components of the geostrophic velocity perpendicular to the ascending and descending track, respectively.
The covariances of the velocity fluctuations , and are then
computed from the 2-year time sériés of u’ and v’ velocity components. The
results are displayed in Fig. 6. It is important to underline that Johnson et al. [13]
estimated that the decorrelation times from u' and v' are 31 and 14 days, respectively. This gives high reliability to results from analysis of T/P crossover, being
the maximum delay between the two passes at the crossover less than 10 days.
The patterns of , and (see Fig. 6) show a fair geographical
cohérence with scales of hundreds of kilométrés. In several areas, mostly at the
lower latitudes,
exceeds as already noticed [10]. This means that
the mesoscale eddies are strongly anisotropic. The interaction of the mean current with the bottom topography produces a complex pattern of. Relatively
high values of are alearly visible in the area of the Pacific-Antarctic Ridge
and near the Kerguelen Plateau.
The magnitude and the direction of the eddy variability are represented in
Fig. 7 by the variance ellipses. The direction of the axis of principal variability,
measured counterclockwise from east, is:
tand =
on -

where j is the variance along the major axis and is given by
a.. = — (++ J (-)2+4 2
2
while the variance along the minor axis is
u22 = (<«V>2+2) - un.
In the background of Fig. 7 the bottom topography with the main ridges and
shallow plateaus is shown using a gray scale.
An anisotropy flow is represented by elongated ellipses, with the principal
direction of the velocity variance aligned with the direction of the major axis;
ellipses with a major axis oriented toward the northeast quadrant hâve a positive
, while ellipses with a major axis oriented toward the southeast quadrant
hâve a négative .
In Fig. 7 distinct anisotropic variability is most évident in the high eddy
régions of the Agulhas Retroflection and Southwest of the Atlantic région.

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