物理
谱线
碰撞
吸收光谱法
吸收(声学)
天体物理学
原子物理学
核物理学
天文
光学
计算机安全
计算机科学
作者
Ryan Johnson,P. F. Bernath,Brant Billinghurst,Jianbao Zhao
标识
DOI:10.3847/1538-4357/ada24a
摘要
Abstract Collision-induced spectra are essential for radiative transfer modeling of Titan's atmosphere. We present experimental spectra of nitrogen–methane mixtures with an accompanying fit of N 2 -CH 4 collision-induced absorption in the 30–400 cm −1 region at about 130 K. We found a peak absorption of 2.30 × 10 −5 cm −1 amagat −2 at 75 cm −1 and a secondary peak of 1.35 × 10 −5 cm −1 amagat −2 at 206.5 cm −1 , which agrees with previous studies. Our work does not support the suggestion that N 2 -CH 4 CIA in the far-infrared should be increased by about 50%, as suggested by spectroscopic modeling of Titan using data from A. Borysow & C. Tang.
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