  The goal of this paper is to describe in mathematical terms the effect on the
ocean circulation of a random stationary wind stress at the surface of the
ocean. In order to avoid singular behaviour, non-resonance hypotheses are
introduced, which ensure that the time frequencies of the wind-stress are
different from that of the Earth rotation. We prove a convergence result for a
three-dimensional Navier-Stokes-Coriolis system in a bounded domain, in the
asymptotic of fast rotation and vanishing vertical viscosity, and we exhibit
some random and stationary boundary layer profiles. At last, an average
equation is derived for the limit system in the case of the non-resonant torus.
