旋转带下的CO-Ar连续体:超级洛伦兹翼是否参与其中?
Aleksandra O Koroleva1, Tatyana A Galanina1, Maksim A Koshelev1
1A. V. Gaponov-Grekhov Institute of Applied Physics of the Russian Academy of Sciences, 46 Ulyanov Street, Nizhny Novgorod 603950, Russia. koral@ipfran.ru.
Physical chemistry chemical physics : PCCP
|June 16, 2025
概括
一氧化碳- (CO-Ar) 连续吸收在远红外测量. 这些结果与双分子吸收模型一致,解释了连续性的起源和强度耗尽效应.
科学领域:
- 频谱学是一种光谱学.
- 分子物理学 分子物理学
- 天体物理学 天体物理学
背景情况:
- 气体混合中的连续性吸收对于大气和天体物理学研究至关重要.
- 了解CO-Ar连续吸收,可以了解分子相互作用.
研究的目的:
- 为了检索和分析CO-Ar连续吸收光谱.
- 验证现有的双分子吸收模型并提出新的模型.
主要方法:
- 富里埃变换光谱在远红外 (40-160厘米-1).
- 使用同步子辐射作为源.
- 高分辨率光谱分析和与低分辨率数据的比较.
主要成果:
- 成功获得了连续压力依赖.
- 高分辨率和低分辨率连续测量显示一致性.
- 观察到的连续性与双分子吸收模型的预测相匹配.
结论:
- 采用第二个病毒系数的双分子吸收模型准确地描述了CO-Ar连续吸收.
- 提出了一种半实证的远翼吸收模型,考虑碰撞持续时间,并通过实验数据进行验证.
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