Prediction of the flow in the cavity between a rotating cone and an ou
ter stationary cone with and without throughflow is considered. A mome
ntum-integral method and a finite difference method for solution of th
e Reynolds-averaged Navier-Stokes equations with a mixing-length model
of turbulence are applied. These two methods have previously been val
idated for flow between corotating and rotor-stator disk systems, but
have not been properly tested for conical systems. Both methods have b
een evaluated by comparing predictions with the experimental measureme
nts of other workers. There is good agreement for cone half-angles gre
ater than or equal to 60 deg but discrepancies are evident for smaller
angles. ''Taylor-type'' vortices, the existence of which has been pos
tulated by other workers and which are not captured by the present ste
ady, axisymmetric models, may contribute to these discrepancies.