It is shown that the symmetry properties of barotropic nonlinear wind driven ocean circulation, as presented in the numerical simulations of Veronis (1966a, b), can easily be derived analytically for large Ekman number, the so-called “small beta regime”, and for any strength of the nonlinearity, by a perturbation expansion in the inverse Ekman number. The solution is a superposition of a vorticity monopole, dipole and quadrupole, the symmetry properties of which are qualitatively the same as those of the Veronis' sequence. It is also shown that the Veronis' sequence does not lead to the inertial Fofonoff (1954) mode, but that the latter is the limit of another sequence in the parameter plane spanned by the Rossby and Ekman numbers.