“…However, this approach can be used only for axial §ight conditions and 3D effects, such as blade tip vortices, are not represented. Another way to model the §ow in the Fenestron consists in solving Navier Stokes equations on a 2D-axisymmetric shroud and by modeling the fan as a fully coupled, time-averaged momentum source term in the momentum equation [7]. While numerical predictions were in good agreement with measurements in the collector area, the pressure distribution was not accurately estimated in the blade region [7].…”