Pressure distributions over a dual cavity cascade were studied at supersoni
c speeds of Mach 1.5 and 2.5. The study was performed through numerical mod
elling and results compared with model measurements. The Reynolds-averaged
Navier-Stokes equations were solved using a finite-volume algorithm in whic
h the inviscid cell interface fluxes were estimated using Poe's approximate
Riemann solver with a second-order extension, and turbulence was modelled
using a two-equation k-omega model with compressibility corrections. Two te
st configurations were selected: (1) a length-to-depth ratio L/D = 1 cavity
followed by another L/D = 1 cavity, and (2) an L/D = 3 cavity followed by
an L/D = 1 cavity. The prediction was compared with that of a single cavity
of the same L/D. It was found that the pressure field around the L/D = 1 c
avity was substantially modified by a preceding L/D = 3 cavity, Changes in
the pressure and pressure drag coefficient were observed. The study clarifi
ed some earlier observations of unsteady modes over a dual cavity cascade,
and confirmed model measurements of the pressure fluctuation under a number
of flow and geometry conditions.