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Effects of back pressure perturbation on shock train oscillations in a rectangular duct
- Source :
- Acta Astronautica. 179:525-535
- Publication Year :
- 2021
- Publisher :
- Elsevier BV, 2021.
-
Abstract
- The nature of flow field inside the scramjet engine consists of shock-shock interaction and the shock boundary layer interaction. For a sustained combustion, a device called isolator plays a critical role in providing adequate pressure to the combustion chamber by a series of bifurcated shock waves called “shock train”. A small downstream pressure perturbation can cause upstream movement of this shock train and results in engine unstart condition. The propagation speed of downstream disturbance can influence the shock train oscillation. In the present study, computational fluid dynamics analysis is conducted to understand the oscillatory characteristic of shock train in a rectangular duct at M =1.75. The impact of downstream perturbation frequency (f b = 10 – 50 Hz) and the amplitude (A = 0.01 – 0.1) are simulated and discussed. The presence of low-frequency oscillation is observed without back pressure perturbation. The downstream pressure perturbation has a noticeable effect on the shock train excursion length i.e., the maximum upstream to downstream distance moved by shock train. The increase in perturbation frequency leads to decrease in disturbance propagation speed. Similarly, the propagation speed increases with the increase in the perturbation amplitude.
- Subjects :
- Physics
Shock wave
020301 aerospace & aeronautics
Oscillation
Back pressure
Astrophysics::High Energy Astrophysical Phenomena
Aerospace Engineering
02 engineering and technology
Mechanics
Unstart
01 natural sciences
Boundary layer
Amplitude
0203 mechanical engineering
0103 physical sciences
Duct (flow)
Combustion chamber
010303 astronomy & astrophysics
Subjects
Details
- ISSN :
- 00945765
- Volume :
- 179
- Database :
- OpenAIRE
- Journal :
- Acta Astronautica
- Accession number :
- edsair.doi...........22572d0885425d62f53dce102dd72606
- Full Text :
- https://doi.org/10.1016/j.actaastro.2020.11.057