Making use of a simple two-layer model, we analyze the impact or freshwater
forcing on the thermohaline circulation. We consider the forward-type circ
ulation dominated by thermal forcing, implying that the freshwater forcing
acts to reduce the density contrast associated with the equator-to-pole tem
perature contrast prescribed in the model. The system is described by two v
ariables: the depth of the upper layer (H) and the density contrast between
the upper and lower layer Delta rho, which decreases with salinity contras
t. The rate of poleward flow of light Surface water and the diapycnal flow
(i.e.. upwelling) driven by widespread small-scale mixing are both modeled
in terms of H and Delta rho Steady states of thermohaline circulation are f
ound when these two flows are equal. The representation of the diapycnal fl
ow {M-D} is instrumental for the dynamics of the system. We present equally
plausible examples of a physically based representation of M-D, for which
the thermohaline circulation either decreases or increases with density con
trast. In the latter case. contrary to the traditional wisdom, the freshwat
er forcing amplifies the circulation and there exists a thermally dominated
equilibrium for arbitrary intensity of freshwater forcing, Here, Stommel's
famous feedback between circulation and salinity contrast is changed from
a positive to a negative feedback. The interaction of such a freshwater boo
sted thermohaline circulation with the climate system is fundamentally, dif
ferent from what is commonly assumed, an issue which is briefly addressed.