The stability of the thermohaline circulation is investigated using an ocea
n general circulation model coupled to a simple atmospheric model. The atmo
spheric model is so developed that it represents the wind stress and the fr
eshwater flux more realistically than existing energy balance models. The c
oupled model can reproduce the realistic deep ocean circulation without any
flux adjustment. Effects of the wind stress and the vertical diffusion on
the thermohaline circulation are studied by conducting various experiments
with the coupled model. The Ekman upwelling between 60 degreesN and 90 degr
eesN brings up salt to the sea surface, while the compensation flow of the
Ekman transport and the wind-driven gyro circulation between 30 degreesN an
d 60 degreesN carry salt horizontally to the high latitudes. By carrying ou
t experiments where the wind stress is completely or partly removed, it is
demonstrated that either of the vertical or the horizontal salt transport p
revents the halocline formation at high latitudes and maintains the thermoh
aline circulation. For an experiment in which the vertical diffusivity is e
nhanced at high latitudes, it is shown that the vertical diffusion at high
latitudes also prevents the halocline formation and stabilizes the thermoha
line circulation. It is also shown that the value of the vertical diffusivi
ty at high latitude affects the existence of the multiple equilibria of the
thermohaline circulation.