B. Hackett et Lp. Roed, NUMERICAL MODELING OF THE HALTEN BANK AREA - A VALIDATION-STUDY, Tellus. Series A, Dynamic meteorology and oceanography, 46(2), 1994, pp. 113-133
From observations and simple model simulations, it has been establishe
d that a proper model of the Halten Bank area must, as a minimum, (i)
include the barotropic component and at least one baroclinic component
, (ii) allow shear instabilities to properly grow into eddies, (iii) i
nclude vertical mixing to allow for entrainment of lower layer water m
asses into the upper layer, (iv) allow for advection of density (tempe
rature and salinity) in the upper water masses, and (v) allow the incl
usion of tides. All of these physics factors are included in the mathe
matical formulation of fully three-dimensional numerical ocean models.
Two such models, arbitrarily named the POM model and the SINMOD model
, have been used to simulate the current, salinity and temperature str
ucture in the Halten Bank area for March 1988 and then validated again
st the Norwegian Continental Shelf Experiment 1988 (NORCSEX'88) data s
et. Although the motion in the two models is governed by the same set
of continuous equations, an inspection of the parameterizations and nu
merical methods employed to solve the governing equations reveals that
the SINMOD model should be expected to provide smoother and less ener
getic results than the POM model. It is also speculated that eddy grow
th is inhibited in both models due to (i) the tendency of level models
to create fictitious diapycnal mixing in areas of sloping density sur
faces, and (ii) too coarse resolution. These conclusions are partially
supported by the validation analysis. In order to facilitate a meanin
gful model-model comparison and validation. specific products were pro
vided by careful analyses of both data and model results in accordance
with a preselected hierarchic set of comparison criteria. The criteri
a focus on mean circulation patterns and horizontal and vertical distr
ibutions. The analyses reveal that the most probable limitation inhibi
ting the models in reproducing the observed structures is the lack of
horizontal resolution. The chosen grid mesh size (4 km) only barely re
solves the eddy scale dictated by the Rossby radius of deformation, th
us inhibiting eddy growth due to shear instabilities. Further, both th
is and earlier studies conclude that it is an open question how comple
x a model needs to be to be able to simulate the observed structure to
a satisfactory degree.