2016
DOI: 10.2514/1.j054298
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Investigation of Unsteady Edney Type IV and VII Shock–Shock Interactions

Abstract: Edney type IV and type VII shock-shock interactions are complex hypersonic flow phenomena. They are characterized by a supersonic jet that reaches far into the flowfield. An experimental investigation of the inner jet structure is difficult, especially in cases where the jet is subject to high-frequency unsteady movements. The present paper provides insight into the jet structure and its movement by means of a highly resolved computational fluid dynamics analysis in thermochemical nonequilibrium that significa… Show more

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Cited by 24 publications
(12 citation statements)
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“…A number of studies have been conducted to study the flow pattern (cf. Frame & Lewis 1997; Windisch, Reinartz & Müller 2016), transition between various flow patterns (cf. Bramlette 1974), heat load (cf.…”
Section: Introductionmentioning
confidence: 99%
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“…A number of studies have been conducted to study the flow pattern (cf. Frame & Lewis 1997; Windisch, Reinartz & Müller 2016), transition between various flow patterns (cf. Bramlette 1974), heat load (cf.…”
Section: Introductionmentioning
confidence: 99%
“…1988; Gaitonde & Shang 1995; Chu & Lu 2012; Windisch et al. 2016; Khatt & Jagadeesh 2018). See the review of Grasso et al.…”
Section: Introductionmentioning
confidence: 99%
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“…Despite the extensive work done on CO 2 hypersonic flows and its nonequilibrium physics, the literature discussing shock interaction patterns for this gas mixture is scarce to the best of the authors' knowledge. Windisch et al [13] simulated the impingement of an oblique shock on a bow shock in front of a cylinder in a CO2-dominated flow, from which a type VII interaction pattern was obtained. A comparison with the same test-case but considering instead an N 2 mixture revealed that the post-shock temperatures were significantly lower for the gas model of the Martian atmosphere, resulting in a higher fluid density and a much smaller shock stand-off distance.…”
Section: Introductionmentioning
confidence: 99%
“…To the best of the authors' knowledge, the literature discussing the identification of shock wave interference patterns and the associated aerothermal loads in the case of CO 2dominated flows is still not fully consolidated. Windisch et al [19] simulated the intersection between an oblique shock and a bow shock in front of a cylinder with a CO 2dominated flow and observed the type VII interaction. A comparison with the same test case but considering instead a N 2 mixture revealed that the post-shock temperatures were significantly lower for the gas model of the Martian atmosphere, resulting in a higher fluid density and a much smaller shock stand-off distance.…”
mentioning
confidence: 99%