TY - GEN
T1 - Numerical Investigation of Laminar-Turbulent Boundary-Layer Transition for an Ogive Geometry at Mach 7
T2 - AIAA AVIATION FORUM AND ASCEND, 2025
AU - Perez, Hannah
AU - Hader, Christoph
AU - Fasel, Hermann F.
N1 - Publisher Copyright:
© 2025, American Institute of Aeronautics and Astronautics Inc, AIAA. All rights reserved.
PY - 2025
Y1 - 2025
N2 - Numerical investigations were carried out for an ogive geometry with a blunted nose tip at zero angle of attack for atmospheric flight conditions at M = 7.1. These investigations are compared to those for the flow conditions of the hypersonic wind tunnel (H2K) experiments conducted by the German Aerospace Center (DLR), also at M = 7.1. For this comparison, the Mach and unit Reynolds numbers for both flight and wind tunnel conditions are the same allowing for a direct comparison of how a change from wind tunnel to flight conditions affects the linear and nonlinear transition regimes. Linear Stability Theory (LST) calculations revealed that while both first and second mode waves experience significant amplification under wind tunnel conditions, only second mode waves are present under flight conditions. Similar to the investigations for the wind tunnel conditions, primary wave saturation and transition onset calculations were carried out for the flight conditions to determine whether large amplitude second mode waves can reach amplitudes sufficient for transition onset. Secondary instability calculations showed that the so-called fundamental resonance leads to strong secondary amplification, making this a relevant mechanism that could lead to transition for the ogive geometry under atmospheric flight conditions. Based on the primary and secondary instability investigations, high-resolution "controlled" transition simulations have been set up and are currently underway.
AB - Numerical investigations were carried out for an ogive geometry with a blunted nose tip at zero angle of attack for atmospheric flight conditions at M = 7.1. These investigations are compared to those for the flow conditions of the hypersonic wind tunnel (H2K) experiments conducted by the German Aerospace Center (DLR), also at M = 7.1. For this comparison, the Mach and unit Reynolds numbers for both flight and wind tunnel conditions are the same allowing for a direct comparison of how a change from wind tunnel to flight conditions affects the linear and nonlinear transition regimes. Linear Stability Theory (LST) calculations revealed that while both first and second mode waves experience significant amplification under wind tunnel conditions, only second mode waves are present under flight conditions. Similar to the investigations for the wind tunnel conditions, primary wave saturation and transition onset calculations were carried out for the flight conditions to determine whether large amplitude second mode waves can reach amplitudes sufficient for transition onset. Secondary instability calculations showed that the so-called fundamental resonance leads to strong secondary amplification, making this a relevant mechanism that could lead to transition for the ogive geometry under atmospheric flight conditions. Based on the primary and secondary instability investigations, high-resolution "controlled" transition simulations have been set up and are currently underway.
KW - Angle of Attack
KW - Direct Numerical Simulation
KW - Freestream Mach Number
KW - German Aerospace Center
KW - High Speed Flows
KW - Hypersonic International Flight Research Experimentation
KW - Hypersonic Wind Tunnels
KW - Laminar Turbulent Transition
KW - Numerical Investigation
KW - Wavenumber
UR - https://www.scopus.com/pages/publications/105018111665
UR - https://www.scopus.com/pages/publications/105018111665#tab=citedBy
U2 - 10.2514/6.2025-3602
DO - 10.2514/6.2025-3602
M3 - Conference contribution
AN - SCOPUS:105018111665
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
Y2 - 21 July 2025 through 25 July 2025
ER -