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Next: 3.15.3 Discrete Numerical Configuration
Up: 3.15 Centennial Time Scale
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Contents
3.15.2 Overview
This example experiment demonstrates using the MITgcm to simulate
the planetary ocean circulation. The simulation is configured
with realistic geography and bathymetry on a
spherical polar grid.
Twenty vertical layers are used in the vertical, ranging in thickness
from
at the surface to
at depth,
giving a maximum model depth of
.
At this resolution, the configuration
can be integrated forward for thousands of years on a single
processor desktop computer.
The model is forced with climatological wind stress data and surface
flux data from Da Silva [10]. Climatological data
from Levitus [36] is used to initialize the model hydrography.
Levitus data is also used throughout the calculation
to derive air-sea fluxes of heat at the ocean surface.
These fluxes are combined with climatological estimates of
surface heat flux and fresh water, resulting in a mixed boundary
condition of the style described in Haney [25].
Altogether, this yields the following forcing applied
in the model surface layer.
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(3.96) |
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(3.97) |
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(3.98) |
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(3.99) |
where
,
,
,
are the forcing terms in the zonal and meridional
momentum and in the potential temperature and salinity
equations respectively.
The term
represents the top ocean layer thickness.
It is used in conjunction with the reference density,
(here set to
), the
reference salinity, (here set to 35ppt),
and a specific heat capacity to convert
wind-stress fluxes given in
,
The configuration is illustrated in figure .
Next: 3.15.3 Discrete Numerical Configuration
Up: 3.15 Centennial Time Scale
Previous: 3.15.1 Introduction
Contents
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