Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8055672 | Acta Astronautica | 2018 | 30 Pages |
Abstract
The deceleration of a supersonic flow to the subsonic regime inside a high-speed engine occurs through a series of shock waves, known as a shock train. The generation of such a flow structure is due to the interaction between the shock waves and the boundary layer inside a long and narrow duct. The understanding of the physics governing the shock train is vital for the improvement of the design of high-speed engines and the development of flow control strategies. The present paper analyses the sensitivity of the shock train configuration to a back-pressure variation. The complex characteristics of the shock train at an inflow Mach number Mâ¯=â¯2 in a channel of constant height are investigated with two-dimensional RANS equations closed by the Wilcox k-Ï turbulence model. Under a sinusoidal back-pressure variation, the simulated results indicate that the shock train executes a motion around its mean position that deviates from a perfect sinusoidal profile with variation in oscillation amplitude, frequency, and whether the pressure is first increased or decreased.
Related Topics
Physical Sciences and Engineering
Engineering
Aerospace Engineering
Authors
F. Gnani, H. Zare-Behtash, C. White, K. Kontis,