操作 OH 的光谱成像 A2Σ+ → X2Π 1D 在高压甲火焰中的排放
Joshua B Sinrud1,2, Rachel A Schwind3, Brahm N Dean1
1Department of Chemistry and Biochemistry, Montana State University, Bozeman, Montana 59717, United States.
The journal of physical chemistry. A
|December 31, 2025
概括
高压甲火焰中激发的基 (OH*) 排放在氧化和惰性环境之间存在显著差异. OH*排放在空气中持续存在,但在中突然减少,为燃烧模式提供了洞察力.
科学领域:
- 燃烧科学 燃烧科学
- 频谱学是一种光谱学.
- 化学工程是化学工程的重要组成部分.
背景情况:
- 甲 (NM) 燃烧对于单推进剂应用至关重要.
- 了解像OH*这样的激发物种是建模燃烧过程的关键.
- 高压燃烧环境对诊断提出了独特的挑战.
研究的目的:
- 为了在高压 (34 bar) 下在甲火焰中空间分离激发的OH (OH*) 排放.
- 调查氧化与惰性环境对OH*排放的影响.
- 为计算式燃烧模型提供基准.
主要方法:
- 利用光学发射光谱来捕获空间分辨率的光谱图像.
- 从OH A2Σ+ → X2Π放松分析的辐射光谱.
- 沿着火焰轴计算的振动和旋转温度.
主要成果:
- 在空气中的甲火焰中,空间分辨的OH*排放持续存在.
- 在惰性 (N2) 大气中,OH* 排放在甲火焰附近迅速减少.
- OH*的旋转温度看起来是热化的,而振动温度表明了过量的能量.
- 根据振动温度推断OH*的形成路径 (化学与热).
结论:
- 环境对高压甲火焰中的OH*排放特征产生重大影响.
- 这些发现为验证单推进器燃烧模型提供了关键数据.
- 在OH*中过多的振动能量表明火焰内部存在复杂的形成动态.
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