Effect of the axial cavity with an opposing high-pressure jet combination in a Mach 6 flow condition
| Autor: | Gopalan Jagadeesh, B. Sudarshan, Srisha M. V. Rao, S. Saravanan |
|---|---|
| Rok vydání: | 2021 |
| Předmět: |
Overall pressure ratio
020301 aerospace & aeronautics Hypersonic speed Materials science Astrophysics::High Energy Astrophysical Phenomena Expansion tunnel Hypersonic flight Aerospace Engineering 02 engineering and technology Mechanics 01 natural sciences Schlieren imaging symbols.namesake 0203 mechanical engineering Heat flux Mach number 0103 physical sciences Heat transfer symbols 010303 astronomy & astrophysics |
| Zdroj: | Acta Astronautica. 178:335-348 |
| ISSN: | 0094-5765 |
| DOI: | 10.1016/j.actaastro.2020.09.021 |
| Popis: | Flow control techniques mitigating the aerothermal heating over bodies are essential for long-duration hypersonic flight. The combination technique of a nose cavity with an opposing jet is exhibited promising effects. There is a lacuna of experimental studies on unsteady aspects of the flow and the heat transfer effects within the cavity. In the current study, we investigated the heat transfer variations and nature of shock around a blunt body with a cylindrical and parabolic cavity geometries combined with opposing jet. Experiments are conducted in the hypersonic shock tunnel for a flow Mach number of 6 for an opposing jet pressure ratio of 18. Time-resolved high-speed schlieren imaging and heat flux measurements over the model surface and within the cavity are carried out. The cavity flow is established by verifying the measured heat flux, pressure, and shock oscillation results. The combination technique shows a significant reduction of heat transfer and flow oscillations in comparison to the nose cavity technique. Notably, the parabolic cavity with the opposing jet showed about a 33% reduction of surface heat flux and a 43% reduction in flow oscillations. The substantial increase of heat flux due to the shock interaction is noted on the nose surface for a cylindrical cavity geometry, and such effect was not prevalent in the case of flow with parabolic cavity geometry. |
| Databáze: | OpenAIRE |
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