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Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. / Istomin, V. A. ; Kustova, E. V. ; Prutko, K. A. .

In: Vestnik St. Petersburg University: Mathematics, Vol. 55, No. 4, 12.2022, p. 461-470.

Research output: Contribution to journalArticlepeer-review

Harvard

Istomin, VA, Kustova, EV & Prutko, KA 2022, 'Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves', Vestnik St. Petersburg University: Mathematics, vol. 55, no. 4, pp. 461-470.

APA

Istomin, V. A., Kustova, E. V., & Prutko, K. A. (2022). Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. Vestnik St. Petersburg University: Mathematics, 55(4), 461-470.

Vancouver

Istomin VA, Kustova EV, Prutko KA. Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. Vestnik St. Petersburg University: Mathematics. 2022 Dec;55(4):461-470.

Author

Istomin, V. A. ; Kustova, E. V. ; Prutko, K. A. . / Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. In: Vestnik St. Petersburg University: Mathematics. 2022 ; Vol. 55, No. 4. pp. 461-470.

BibTeX

@article{f4d6ef03de0440ceb2fccf91ae29f2bd,
title = "Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves",
abstract = "State-to-state and two-temperature theoretical models for high-temperature strongly nonequilibrium reacting air flows and heat and radiative fluxes are developed in the framework of the generalized Chapman–Enskog method. In the theoretical approach, systems of governing equations for coupled fluid dynamics, chemical kinetics, internal energy transitions and radiation are derived; algorithms for calculating the state-to-state transport coefficients are developed and implemented. The proposed models are applied for simulations of planar shock waves in air under high-temperature conditions observed in flight experiments. A nonequilibrium mixture composition, temperatures and pressure profiles are obtained. We demonstrate that flow variables strongly depend on both the applied approach of kinetic theory and choice of the chemical-reaction model: species molar fractions and temperature show significantly different behaviors for the state-to-state and two-temperature simulations. The transport properties and radiative fluxes are calculated as functions of the distance from the shock front. It is found that diffusion provides a major contribution to the total energy flux whereas the role of heat conduction is weak due to compensation effects. We show that under the considered conditions, two-temperature models are not applicable for correct predictions of radiative heating.",
keywords = "state-to-state kinetics, electronic excitation, transport processes, heat flux, radiative flux",
author = "Istomin, {V. A.} and Kustova, {E. V.} and Prutko, {K. A.}",
note = "Istomin, V.A., Kustova, E.V. & Prutko, K.A. Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. Vestnik St.Petersb. Univ.Math. 55, 461–470 (2022). https://doi.org/10.1134/S1063454122040094",
year = "2022",
month = dec,
language = "English",
volume = "55",
pages = "461--470",
journal = "Vestnik St. Petersburg University: Mathematics",
issn = "1063-4541",
publisher = "Pleiades Publishing",
number = "4",

}

RIS

TY - JOUR

T1 - Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves

AU - Istomin, V. A.

AU - Kustova, E. V.

AU - Prutko, K. A.

N1 - Istomin, V.A., Kustova, E.V. & Prutko, K.A. Heat and Radiative Fluxes in Strongly Nonequilibrium Flows Behind Shock Waves. Vestnik St.Petersb. Univ.Math. 55, 461–470 (2022). https://doi.org/10.1134/S1063454122040094

PY - 2022/12

Y1 - 2022/12

N2 - State-to-state and two-temperature theoretical models for high-temperature strongly nonequilibrium reacting air flows and heat and radiative fluxes are developed in the framework of the generalized Chapman–Enskog method. In the theoretical approach, systems of governing equations for coupled fluid dynamics, chemical kinetics, internal energy transitions and radiation are derived; algorithms for calculating the state-to-state transport coefficients are developed and implemented. The proposed models are applied for simulations of planar shock waves in air under high-temperature conditions observed in flight experiments. A nonequilibrium mixture composition, temperatures and pressure profiles are obtained. We demonstrate that flow variables strongly depend on both the applied approach of kinetic theory and choice of the chemical-reaction model: species molar fractions and temperature show significantly different behaviors for the state-to-state and two-temperature simulations. The transport properties and radiative fluxes are calculated as functions of the distance from the shock front. It is found that diffusion provides a major contribution to the total energy flux whereas the role of heat conduction is weak due to compensation effects. We show that under the considered conditions, two-temperature models are not applicable for correct predictions of radiative heating.

AB - State-to-state and two-temperature theoretical models for high-temperature strongly nonequilibrium reacting air flows and heat and radiative fluxes are developed in the framework of the generalized Chapman–Enskog method. In the theoretical approach, systems of governing equations for coupled fluid dynamics, chemical kinetics, internal energy transitions and radiation are derived; algorithms for calculating the state-to-state transport coefficients are developed and implemented. The proposed models are applied for simulations of planar shock waves in air under high-temperature conditions observed in flight experiments. A nonequilibrium mixture composition, temperatures and pressure profiles are obtained. We demonstrate that flow variables strongly depend on both the applied approach of kinetic theory and choice of the chemical-reaction model: species molar fractions and temperature show significantly different behaviors for the state-to-state and two-temperature simulations. The transport properties and radiative fluxes are calculated as functions of the distance from the shock front. It is found that diffusion provides a major contribution to the total energy flux whereas the role of heat conduction is weak due to compensation effects. We show that under the considered conditions, two-temperature models are not applicable for correct predictions of radiative heating.

KW - state-to-state kinetics

KW - electronic excitation

KW - transport processes

KW - heat flux

KW - radiative flux

UR - https://link.springer.com/article/10.1134/S1063454122040094

M3 - Article

VL - 55

SP - 461

EP - 470

JO - Vestnik St. Petersburg University: Mathematics

JF - Vestnik St. Petersburg University: Mathematics

SN - 1063-4541

IS - 4

ER -

ID: 101701921