TY - GEN
T1 - Direct Numerical Simulations of Hypersonic Boundary-Layer Transition for a Sharp Cone at Mach 10
AU - Hurworth, Aleksander
AU - Hader, Christoph
AU - Fasel, Hermann F.
N1 - Publisher Copyright:
© 2022, American Institute of Aeronautics and Astronautics Inc.. All rights reserved.
PY - 2022
Y1 - 2022
N2 - Direct Numerical Simulations (DNS) are carried out to investigate the primary and secondary instability for boundary layers on a straight (right) cone with a 7◦ opening half-angle at Mach 10 and zero angle of attack. The cone geometry of the experiments in the Arnold Engineering Development Complex (AEDC) Hypervelocity Wind Tunnel No. 9 (Tunnel 9) was used for the numerical investigations. Three different unit Reynolds numbers were considered for the primary and secondary instability calculations. As expected, the linear amplification rates and the corresponding N-factors decrease with decreasing unit Reynolds numbers. For all investigated cases the axisymmetric second mode disturbances were the dominant primary linear instability. An investigation of the primary wave saturation amplitudes revealed that the maximum second mode amplitudes depended only weakly on the unit Reynolds number. Secondary instability investigations showed that the wave angle of the secondary disturbance wave resulting in the strongest resonance (largest N-factor after resonance onset) remains largely unaffected by the unit Reynolds number. In addition, the same azimuthal wavenumber range experiences strong secondary instability for the investigated unit Reynolds numbers. Emphasis of the present paper is on the primary and secondary wave regime. Results from high-fidelity DNS of the entire transition process, from the linear stages all the way to complete breakdown, will be presented and discussed in a future paper.
AB - Direct Numerical Simulations (DNS) are carried out to investigate the primary and secondary instability for boundary layers on a straight (right) cone with a 7◦ opening half-angle at Mach 10 and zero angle of attack. The cone geometry of the experiments in the Arnold Engineering Development Complex (AEDC) Hypervelocity Wind Tunnel No. 9 (Tunnel 9) was used for the numerical investigations. Three different unit Reynolds numbers were considered for the primary and secondary instability calculations. As expected, the linear amplification rates and the corresponding N-factors decrease with decreasing unit Reynolds numbers. For all investigated cases the axisymmetric second mode disturbances were the dominant primary linear instability. An investigation of the primary wave saturation amplitudes revealed that the maximum second mode amplitudes depended only weakly on the unit Reynolds number. Secondary instability investigations showed that the wave angle of the secondary disturbance wave resulting in the strongest resonance (largest N-factor after resonance onset) remains largely unaffected by the unit Reynolds number. In addition, the same azimuthal wavenumber range experiences strong secondary instability for the investigated unit Reynolds numbers. Emphasis of the present paper is on the primary and secondary wave regime. Results from high-fidelity DNS of the entire transition process, from the linear stages all the way to complete breakdown, will be presented and discussed in a future paper.
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U2 - 10.2514/6.2022-0945
DO - 10.2514/6.2022-0945
M3 - Conference contribution
AN - SCOPUS:85123440705
SN - 9781624106316
T3 - AIAA Science and Technology Forum and Exposition, AIAA SciTech Forum 2022
BT - AIAA SciTech Forum 2022
PB - American Institute of Aeronautics and Astronautics Inc, AIAA
T2 - AIAA Science and Technology Forum and Exposition, AIAA SciTech Forum 2022
Y2 - 3 January 2022 through 7 January 2022
ER -