A coarse resolution, three-dimensional numerical model is used to study how
external parameters control the existence and strength of equatorially asy
mmetric thermohaline overturning in a large-scale, rotating ocean basin. In
itially, the meridional surface density gradient is directly set to be larg
er in a "dominant" hemisphere than in a "subordinate" hemisphere. The two-h
emisphere system has a broader thermocline and weaker upwelling than the sa
me model with the dominant hemisphere only. This behavior is in accord with
classical scaling arguments, providing that the continuity equation is emp
loyed, rather than the linear vorticity equation.
The dominant overturning cell, analogous to North Atlantic Deep Water forma
tion, is primarily controlled by the surface density contrast in the domina
nt hemisphere, which in turn is largely set by temperature. Consequently, i
n experiments with mixed boundary conditions, the dominant cell strength is
relatively insensitive to the magnitude Q(s) of the salinity forcing. Howe
ver, a, strongly influences subordinate hemisphere properties, including th
e volume transport of a shallow overturning cell and the meridional extent
of a tongue of low-salinity intermediate water reminiscent of Antarctic Int
ermediate Water.
The minimum Q(s) is identified for which the steady, asymmetric how is stab
le; below this value, a steady, equatorially symmetric, temperature-dominat
ed overturning occurs. For high salt flux, the asymmetric circulation becom
es oscillatory and eventually gives way to an unsteady, symmetric, salt-dom
inated overturning. For given boundary conditions, it is possible to have a
t least three different asymmetric states, with significantly different lar
ge-scale properties. An expression for the meridional salt transport allows
one to roughly predict the surface salinity and density profile and stabil
ity of the asymmetric state as a function of Q(s) and other external parame
ters.