Nitrogen molecular radiation in hypersonic expanding flow

This study investigates nitrogen molecular radiation in hypersonic expanding flow around a two-dimensional model. Experiments were conducted using the JF-14 shock tunnel in shock tube mode, generating a 3.25 km/s shock wave to create the required flow. A blunt model with a 25-mm nose radius was used to generate the expanding flow. Spatially resolved visible spectra were measured around the model's shoulder. Numerical simulations were then conducted to analyze flow properties and spectral distributions. The results show that the N2 first positive system dominates emissions in the 500–750 nm range. The spectral profiles matched well between experiment and simulation, but predicted intensities were 3–4 times higher, likely due to an overestimation of the excited state density in the model. A detected spectral line near 520 nm, close to the wall, suggests that the predissociation may have been underestimated. This work extends experimental data on hypersonic expanding flow, contributing to an improved understanding of radiation in such flows.

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Publication Details

Journal
Physics of Fluids
Published
2025-02-01
DOI
https://doi.org/10.1063/5.0251388
Citations
4
Primary Topic
Gas Dynamics and Kinetic Theory
Type
article
Field-Weighted Citation Impact
14.91

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article

Nitrogen molecular radiation in hypersonic expanding flow

Tianrui Bai, Senhao Zhang, Xin Lin, Fei Li et al.
4 citations
Physics of Fluids
Gas Dynamics and Kinetic Theory
14.91
article

Nitrogen molecular radiation in hypersonic expanding flow

Tianrui Bai, Senhao Zhang, Xin Lin, Fei Li, Xiaoyuan Zhang, Jiaying Wang, Jinping Li, Shizhong Zhang, Yixin Xu
article en
4 citations

Abstract

This study investigates nitrogen molecular radiation in hypersonic expanding flow around a two-dimensional model. Experiments were conducted using the JF-14 shock tunnel in shock tube mode, generating a 3.25 km/s shock wave to create the required flow. A blunt model with a 25-mm nose radius was used to generate the expanding flow. Spatially resolved visible spectra were measured around the model's shoulder. Numerical simulations were then conducted to analyze flow properties and spectral distributions. The results show that the N2 first positive system dominates emissions in the 500–750 nm range. The spectral profiles matched well between experiment and simulation, but predicted intensities were 3–4 times higher, likely due to an overestimation of the excited state density in the model. A detected spectral line near 520 nm, close to the wall, suggests that the predissociation may have been underestimated. This work extends experimental data on hypersonic expanding flow, contributing to an improved understanding of radiation in such flows.

Physics of FluidsVol. 37(2)
Chinese Academy of Sciences (CN), Jiangsu University of Science and Technology (CN), Institute of Mechanics (CN), University of Chinese Academy of Sciences (CN)
National Natural Science Foundation of China
Openalex Percentile: Top 1%
Gas Dynamics and Kinetic Theory
14.91
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Nitrogen molecular radiation in hypersonic expanding flow — Tianrui Bai, Senhao Zhang, et al. · Physics of Fluids (2025) | TGRS Research Map | TGRS