This paper presents numerical simulations of the unsteady flow interactions between the main annulus and the disc cavity for an axial turbine. The simulations show the influence of the main annulus asymmetries (vane wakes, blade potential effect), and the appearance of rim seal flow instabilities. The generation of secondary frequencies due to non-linear interactions is observed, and the possibility of further low frequency effects and resonance is noted. The computations are compared to experimental results, looking at tracer gas concentration and massflows. Results are further analysed to investigate the influence of the rim seal flow on the blading aerodynamics. The flow that is ejected through the rim seal influences the unsteady flow impinging the blades. The influence of this rim-seal flow is even observed downstream of the blades, where it distorts the radial profile of stagnation temperature. NOMENCLATURE d axial distance between the rows f bld blade passing frequency Ma characteristic Mach number (based on U e ) m c coolant mass-flow m e main-inlet mass-flow P pressure * Address all correspondence to this author.Re x Reynolds number (based on U e and r hub ) r hub hub radius T temperature U c characteristic velocity based on m c U e characteristic velocity based on m e x, r, θ cylindrical coordinates x, y, z cartesian coordinates β relative flow angle in the circumferential direction η isentropic efficiency ϕ sealing efficiency, based on the concentration of coolant flow ψ mass-flow ratio through the rim seal (estimate of ϕ) Π stagnation pressure ratio between main inlet and outlet ρ e characteristic density in the main annulus CFD Computational Fluid Dynamics 0 [subscript] stagnation quantities i and o [subscript] inlet and outlet [superscript] Fourier transform -[superscript] Time average 1