A time-dependent numerical model of a turbulent
Mach 1.5 flow over a rectangular cavity has been developed,
to investigate suppression strategies for its
natural self-sustained instability. This instability adversely
affects the cavity form drag, it produces large-amplitude
pressure oscillations in the enclosure and it
is a source of far-field acoustic radiation.
To suppress the natural flow instability, the leading
edge of the two-dimensional cavity model is fitted with
a simulated air jet that discharges in the downstream
direction. The jet mass flow rate and nozzle depth are
adjusted to attenuate the instability while minimising
the control mass flow rate.
The numerical predictions indicate that, at the selected
inflow conditions, the configurations with the
deepest nozzle (0.75 of the cavity depth) give the most
attenuation of the modelled instability, which is dominated
by the cavity second mode. The jet affects both
the unsteady pressure field and the vorticity distribution
inside the enclosure, which are, together, key
determinants of the cavity leading instability mode
amplitude. The unsteadiness of the pressure field is reduced
by the lifting of the cavity shear layer at the rear
end above the trailing edge. This disrupts the formation
of upstream travelling feed-back pressure waves
and the generation of far-field noise. The deep nozzle
also promotes a downstream bulk flow in the enclosure,
running from the upstream vertical wall to the
downstream one. This flow attenuates the large-scale
clockwise recirculation that is present in the unsuppressed
cavity flow. The same flow alters the top shear
layer vorticity thickness and probably affects the convective
growth of the shear layer cavity second mode.
History
Citation
Proceedings of the 42nd Aerospace Sciences Meeting and Exhibit, Reno, NV, USA, 5-8 January, 2004, pp. 1-10
Published in
Proceedings of the 42nd Aerospace Sciences Meeting and Exhibit
Available date
2008-02-04
Publisher version
http://www.aiaa.org/content.cfm?pageid=2
Notes
This paper was published as Proceedings of the 42nd Aerospace Sciences Meeting and Exhibit, Reno, NV, USA, 5-8 January, 2004, pp. 1-10. It is also available from http://www.aiaa.org/content.cfm?pageid=2