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Oxygen, nitrogen and air broadening of HCN spectral lines at terahertz frequencies

机译:太赫兹频率下HCN谱线的氧、氮和空气展宽

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摘要

The room-temperature nitrogen- and oxygen-broadening coefficients of hydrogen cyanide spectral lines have been measured in the 0.5-3THz (17-100cm(-1)) frequency range (purely rotational transitions with 5 <= J <= 36) by a continuous-wave terahertz spectrometer based on a photomixing source. An improved version of the Robert and Bonamy semiclassical formalism has been used to calculate the oxygen-broadening coefficients and resulted in a good agreement with these measurements. The nitrogen and oxygen data are combined to provide the air-broadening coefficients as used by the HITRAN database. A significant difference is observed between the measured and tabulated values for transitions with high values of the rotational quantum number. A new polynomial representation is suggested for inclusion in HITRAN. A similar polynomial expression has been derived for the nitrogen broadening to aid the studies of Titan's atmosphere.
机译:氰化氢光谱线的室温氮和氧展宽系数在0.5-3THz(17-100cm(-1))频率范围内(纯旋转跃迁,5 <= J <= 36)通过基于光混合源的连续波太赫兹光谱仪测量。Robert 和 Bonamy 半经典形式主义的改进版本已被用于计算氧展宽系数,并与这些测量结果非常吻合。氮气和氧气数据相结合,提供HITRAN数据库使用的空气展宽系数。在旋转量子数值较高的跃迁的测量值和表格值之间观察到显著差异。建议在HITRAN中包含一种新的多项式表示。对于氮的展宽,已经推导出了类似的多项式表达式,以帮助研究土卫六的大气层。

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