2019
DOI: 10.2514/1.j057775
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Significant Supersonic Modes and the Wall Temperature Effect in Hypersonic Boundary Layers

Abstract: Note the importance of the relative sonic line y s , indicated by My s −1, where My uy − c ay where uy is the local mean flow velocity tangential to the wall, c ω∕ β 2 α 2 p is the disturbance propagation speed (with ω the circular frequency, β the spanwise wave number, and α the streamwise wave number), and ay is the local mean flow speed of sound. The disturbance propagation speed c is constant in the wall-normal direction for the entire disturbance structure at a fixed frequency and location. Between the so… Show more

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Cited by 40 publications
(14 citation statements)
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References 44 publications
(73 reference statements)
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“…Also, as seen in § 4.2.4, the most unstable perturbation is a supersonic mode over a large fraction of the streamwise range. Supersonic modes are known to have a non-exponential decay in the free-stream region (see Knisely & Zhong 2019 a , b , c ), further increasing the amplitude with which they reach the shock.…”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…Also, as seen in § 4.2.4, the most unstable perturbation is a supersonic mode over a large fraction of the streamwise range. Supersonic modes are known to have a non-exponential decay in the free-stream region (see Knisely & Zhong 2019 a , b , c ), further increasing the amplitude with which they reach the shock.…”
Section: Resultsmentioning
confidence: 99%
“…They also concluded that the second mode's characteristic time scale is much shorter than the dissociation/recombination time. Bitter & Shepherd (2015) performed an extensive parametric study on supersonic modes in TNE conditions (yet with frozen chemistry), being later extended to TCNE conditions by Knisely & Zhong (2019 a , b , c ). Their main finding was that unstable supersonic modes generally appeared as a consequence of highly cooled walls.…”
Section: Introductionmentioning
confidence: 99%
“…At M ∞ = 4.5 and 6, the amplification curves exhibit a kink (indicated by a + symbol in figure 7), at which the decreasing phase speed reaches the value c r = 1 − 1/M ∞ , meaning that the wave travels supersonically relative to the free stream. These features are typical of the so-called supersonic mode (Bitter & Shepherd 2015;Mortensen 2018;Knisely & Zhong 2019a). It is worth pointing out that this mode emerges in a frequency range well above the slow-mode one (which is not the case for the first and second perfect-gas modes).…”
Section: 3mentioning
confidence: 93%
“…Figure 11 presents snapshots of static pressure perturbations p illustrating the strong growth of waves by many orders of magnitudes over a few tens of centimeters only. Pressure oscillations also appear around the sonic line which is often observed and indicative of secondmode transition 27,46 Finally, Fig. 12 quantifies the growth of wall pressure perturbations and provides a comparison with the previously discussed LST results.…”
Section: Excitation and Stability Analysismentioning
confidence: 70%