With the Hamburg geostrophic ocean general circulation model, the temp
oral variation of the angular momentum of the oceans is studied. The i
nput wind stresses consist of climatological winds plus the deviations
of the actual winds 1981-1989. The motion part of the angular momenta
of the two hemispheres resembles the (counter-phase) behaviour of the
corresponding atmospheric angular momentum. The dominating matter par
t however shows no phase shift between the hemispheres. The sum of the
angular momenta of the solid Earth and the atmosphere is deduced from
observations; in principle it should be inversely correlated to the o
ceanic angular momentum. A first attempt to recognize the correlation
between these empirical data and the theoretical values is described.