TY - GEN
T1 - Numerical Simulation of Unstart Processes in an Axisymmetric Scramjet Combustor
AU - Hash, Caleb A.
AU - Drummond, Paige M.
AU - Edwards, Jack R.
AU - Kato, Nozomu
AU - Lee, Tonghun
N1 - Funding Information:
This work is supported by the Air Force Office of Scientific Research under grants FA9550-20-1-0408 and FA9550-21-1-0072, monitored by Dr. Chiping Li. Computer time has been provided by the DoD’s High Performance Computing Modernization Program.
Publisher Copyright:
© 2022, American Institute of Aeronautics and Astronautics Inc.. All rights reserved.
PY - 2022
Y1 - 2022
N2 - Large-eddy simulations of stable and unstable ramjet operational modes are presented for an axisymmetric inlet-isolator-combustor configuration experimentally tested in the University of Illinois’s ACT-II arc-heated combustion tunnel. A 32 species ethylene oxidation mechanism including nitrous oxide formation reactions is used in the calculations. Conjugate heat-transfer models based on an assumed penetration depth of the applied heating load are used to account for localized wall heating during the short durations (~0.2 to 0.3 s) of the parts of the experiments simulated in this work. The results show a marked sensitivity to trace levels of atomic oxygen (~1% by mass) in the free stream – these trace levels are a consequence of the arc-heating process at ~1 bar pressure and the use of baffles to enhance mixing of oxygen with arc-heated nitrogen. With 1% atomic oxygen in the free stream, a jet-wake stabilized, partially-premixed flame structure emerges during thermal-throat ramjet operation at an equivalence ratio of 1.24, in accord with available experimental pressure and imaging measurements. Simulations of unstable ram-mode operation leading to inlet unstart at an equivalence ratio of 1.97 indicate a sensitivity to the thermal-wall boundary condition, the ignition method, and the free-stream composition. A reduction in atomic oxygen concentration to 0.8% by mass yields good agreement with the experimentally-observed shock-train propagation speed. Both the computational and experimental results indicate that the shock train accelerates before being disgorged from the inlet. This acceleration stems from a rapid increase in the sizes of regions of low speed, sometimes separated flow behind Mach disks that form as the shock train proceeds upstream.
AB - Large-eddy simulations of stable and unstable ramjet operational modes are presented for an axisymmetric inlet-isolator-combustor configuration experimentally tested in the University of Illinois’s ACT-II arc-heated combustion tunnel. A 32 species ethylene oxidation mechanism including nitrous oxide formation reactions is used in the calculations. Conjugate heat-transfer models based on an assumed penetration depth of the applied heating load are used to account for localized wall heating during the short durations (~0.2 to 0.3 s) of the parts of the experiments simulated in this work. The results show a marked sensitivity to trace levels of atomic oxygen (~1% by mass) in the free stream – these trace levels are a consequence of the arc-heating process at ~1 bar pressure and the use of baffles to enhance mixing of oxygen with arc-heated nitrogen. With 1% atomic oxygen in the free stream, a jet-wake stabilized, partially-premixed flame structure emerges during thermal-throat ramjet operation at an equivalence ratio of 1.24, in accord with available experimental pressure and imaging measurements. Simulations of unstable ram-mode operation leading to inlet unstart at an equivalence ratio of 1.97 indicate a sensitivity to the thermal-wall boundary condition, the ignition method, and the free-stream composition. A reduction in atomic oxygen concentration to 0.8% by mass yields good agreement with the experimentally-observed shock-train propagation speed. Both the computational and experimental results indicate that the shock train accelerates before being disgorged from the inlet. This acceleration stems from a rapid increase in the sizes of regions of low speed, sometimes separated flow behind Mach disks that form as the shock train proceeds upstream.
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U2 - 10.2514/6.2022-1849
DO - 10.2514/6.2022-1849
M3 - Conference contribution
AN - SCOPUS:85123592732
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 -