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Models validation and code profiling in state-to-state simulations of shock heated air flows. / Campoli, L.; Kunova, O.; Kustova, E.; Melnik, M.
In: Acta Astronautica, Vol. 175, 10.2020, p. 493-509.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - Models validation and code profiling in state-to-state simulations of shock heated air flows
AU - Campoli, L.
AU - Kunova, O.
AU - Kustova, E.
AU - Melnik, M.
PY - 2020/10
Y1 - 2020/10
N2 - The objective of this study is to examine various combinations of vibration-chemical coupling models in high-temperature air and oxygen flows behind shock waves. Simulations are carried out in the frame of the state-to-state approach for detailed vibrational and chemical kinetics in the Euler approximation. Great variety of state-resolved models for the rate coefficients of vibrational energy transitions and chemical reactions are assessed and validated against experimental data; among them are first-order perturbation (SSH) and forced harmonic oscillator (FHO) models; well-known Marrone–Treanor dissociation model with parameters either obtained empirically or by fitting quasiclassical trajectory calculations; new models for state-specific Zeldovich reactions. To validate the models, the results of numerical flow simulations are compared with experimental investigations in a wide range of initial mixture compositions and shock wave velocities. Among numerous model variants, a few models providing the best agreement with the experimental data on the vibrational temperature in oxygen flows and measured NO radiation in air flows are recommended for different sets of free stream conditions. The impact of NO excited states produced in Zeldovich reactions is evaluated; it is shown that neglecting the vibrational excitation of NO molecules may lead to significantly underpredicted maximum of NO number density. In the framework of the code performance study, Matlab and Fortran implementations were compared, the most significant bottlenecks procedures were identified by profiling analysis, and remarkable speed-up was achieved by code optimisation.
AB - The objective of this study is to examine various combinations of vibration-chemical coupling models in high-temperature air and oxygen flows behind shock waves. Simulations are carried out in the frame of the state-to-state approach for detailed vibrational and chemical kinetics in the Euler approximation. Great variety of state-resolved models for the rate coefficients of vibrational energy transitions and chemical reactions are assessed and validated against experimental data; among them are first-order perturbation (SSH) and forced harmonic oscillator (FHO) models; well-known Marrone–Treanor dissociation model with parameters either obtained empirically or by fitting quasiclassical trajectory calculations; new models for state-specific Zeldovich reactions. To validate the models, the results of numerical flow simulations are compared with experimental investigations in a wide range of initial mixture compositions and shock wave velocities. Among numerous model variants, a few models providing the best agreement with the experimental data on the vibrational temperature in oxygen flows and measured NO radiation in air flows are recommended for different sets of free stream conditions. The impact of NO excited states produced in Zeldovich reactions is evaluated; it is shown that neglecting the vibrational excitation of NO molecules may lead to significantly underpredicted maximum of NO number density. In the framework of the code performance study, Matlab and Fortran implementations were compared, the most significant bottlenecks procedures were identified by profiling analysis, and remarkable speed-up was achieved by code optimisation.
KW - Code profiling
KW - Model validation
KW - Shock wave
KW - State-resolved reaction rate coefficients
KW - State-to-state flow simulations
KW - Vibration-chemical coupling
UR - http://www.scopus.com/inward/record.url?scp=85086475264&partnerID=8YFLogxK
UR - https://www.mendeley.com/catalogue/310d2e74-0228-3626-b91a-e5a8c290282e/
U2 - 10.1016/j.actaastro.2020.06.008
DO - 10.1016/j.actaastro.2020.06.008
M3 - Article
AN - SCOPUS:85086475264
VL - 175
SP - 493
EP - 509
JO - Acta Astronautica
JF - Acta Astronautica
SN - 0094-5765
ER -
ID: 60217971