TY - GEN
T1 - Controlled Transition Simulations on an Axisymmetric 8-Degree Compression Ramp at Mach 5
AU - Tsakagiannis, Vasilis
AU - Hader, Christoph
AU - Fasel, Hermann F.
N1 - Publisher Copyright: © 2025, American Institute of Aeronautics and Astronautics, Inc. All rights reserved.
PY - 2025
Y1 - 2025
N2 - Numerical investigations are conducted to investigate the transitional shock-boundary-layer interaction (SBLI) on a hollow cylinder flare geometry at Mach 5. The flow conditions are matched as closely as possible to those used in experiments at the Mach 5 Ludwieg Tube (LT5) at the University of Arizona (UA). A variation of the geometry used in the experiments was used for the numerical simulations with a flare angle of 8◦. This case was previously identified as only convectively unstable, with no signs of an absolute/global instability. The linear regime is investigated using local linear stability theory (LST) and low amplitude controlled forcing simulations. An oblique 1st mode/shear-layer mode is found to be amplified for a range of azimuthal wavenumbers. Subsequently, highly resolved direct numerical simulations (DNS) are performed in order to investigate the possibility of an oblique breakdown scenario, dominated by the 1st mode/shear-layer mode. Contours of the azimuthal averaged skin friction over time, show that the separation region for the transitional flow contracts compared to the laminar base flow. Pressure amplitude spectra show the amplification of the nonlinearly generated signature modes, consistent with an oblique breakdown scenario. Time averaged skin-friction coefficient and Stanton number, and their Fourier transformed amplitudes, indicate the formation of streaks that appear already inside the separation bubble. Towards the end of the computational domain, smaller structures can be observed in the instantaneous pseudo-Schlieren contours visualizations indicating that the late nonlinear stages of the transition process have been reached.
AB - Numerical investigations are conducted to investigate the transitional shock-boundary-layer interaction (SBLI) on a hollow cylinder flare geometry at Mach 5. The flow conditions are matched as closely as possible to those used in experiments at the Mach 5 Ludwieg Tube (LT5) at the University of Arizona (UA). A variation of the geometry used in the experiments was used for the numerical simulations with a flare angle of 8◦. This case was previously identified as only convectively unstable, with no signs of an absolute/global instability. The linear regime is investigated using local linear stability theory (LST) and low amplitude controlled forcing simulations. An oblique 1st mode/shear-layer mode is found to be amplified for a range of azimuthal wavenumbers. Subsequently, highly resolved direct numerical simulations (DNS) are performed in order to investigate the possibility of an oblique breakdown scenario, dominated by the 1st mode/shear-layer mode. Contours of the azimuthal averaged skin friction over time, show that the separation region for the transitional flow contracts compared to the laminar base flow. Pressure amplitude spectra show the amplification of the nonlinearly generated signature modes, consistent with an oblique breakdown scenario. Time averaged skin-friction coefficient and Stanton number, and their Fourier transformed amplitudes, indicate the formation of streaks that appear already inside the separation bubble. Towards the end of the computational domain, smaller structures can be observed in the instantaneous pseudo-Schlieren contours visualizations indicating that the late nonlinear stages of the transition process have been reached.
KW - Adverse Pressure Gradient
KW - Amplitude Control
KW - Direct Numerical Simulation
KW - Gortler Vortices
KW - Laminar Turbulent Transition
KW - Mach Numbers
KW - Numerical Simulation
KW - Skin Friction Coefficient
KW - Transitional Flow
KW - Traveling Wave
UR - https://www.scopus.com/pages/publications/105018044181
UR - https://www.scopus.com/pages/publications/105018044181#tab=citedBy
U2 - 10.2514/6.2025-3605
DO - 10.2514/6.2025-3605
M3 - Conference contribution
SN - 9781624107382
T3 - AIAA Aviation Forum and ASCEND, 2025
BT - AIAA AVIATION FORUM AND ASCEND, 2025
PB - American Institute of Aeronautics and Astronautics Inc, AIAA
T2 - AIAA AVIATION FORUM AND ASCEND, 2025
Y2 - 21 July 2025 through 25 July 2025
ER -