Abstract:
A simple quasi-two dimensional dynamical model of Thermohaline circulation
(THC) is developed, assuming that the mixing only occurs near western and eastern
boundary layers. When the surface density is prescribed, the climatically important
quantities, such as the strength of overturning and meridional heat transport, are related
to the zonal integral over the vigorously mixing regions and scaled as (KvΔx )2/3.
The numerical results suggest that the density difference between eastern and western
boundaries play an important role in the meridional overturning. The eastern boundary
is characterized by the upwelling on top of downwelling. The western boundary
layer is featured by the universal upwelling. The inefficiency of diffusion heat transport
accounts for the narrowness of sinking region and shallowness of overturning
cell in one-hemisphere. The experiments with other surface boundary conditions are
also explored. The circulation patterns obtained are similar under various surface
temperature distributions, suggesting these are very robust features of THC.
The role of boundary mixing is further explored in global ocean. The 2 1/2 dynamical
model is extended to two-hemisphere ocean. Additional dynamics such as
Rayleigh friction and abyssal water properties are taken into account. A set of complicated
governing equations are derived and numerically solved to obtain steady state
solution. The basic circulation features are revealed in our dynamical model. An
equtorially asymmetric meridional circulation is observed due to small perturbation
at the surface temperature in the high latitude. The density differences between eastern
and western boundaries are distinct in both hemispheres. This is achieved during
the spin-up process.
Although the dynamical model results agree well with OGCM results in one-hemisphere,
several important dynamics are lacking and exposed in two-hemisphere
experiments. We need to consider horizontal advection terms which will effectively
advect positive density anomalies across the equator and form the deep water for the
entire system.
