Journal of Quantitative Spectroscopy and Radiative Transfer ( IF 2.3 ) Pub Date : 2022-06-17 , DOI: 10.1016/j.jqsrt.2022.108284 Jason J. Sorensen , Peter F. Bernath , Ryan M. Johnson , Randika Dodangodage , W. Doug Cameron , Keith LaBelle
The infrared absorption cross sections of pure n-butane, n-pentane, cyclopentane and cyclohexane have been measured in the 3.3 µm region (and 6.8 µm region for cyclopentane) by high resolution Fourier transform spectroscopy. The samples had temperatures of 294 K and 230 K for n-butane, 294 K and 218 K for n-pentane, 296 K and 235 K for cyclopentane, and 294 K and 222 K for cyclohexane. These spectra are important for molecular identification in extraterrestrial environments such as Saturn's moon Titan, giant planets and exoplanets. All spectra are provided as data point files.
中文翻译:
正丁烷、正戊烷、环戊烷和环己烷的吸收截面
纯正丁烷、正戊烷、环戊烷和环己烷的红外吸收截面已通过高分辨率傅里叶变换光谱在 3.3 µm 区域(环戊烷为 6.8 µm 区域)测量。样品的正丁烷温度为 294 K 和 230 K ,正戊烷温度为 294 K 和 218 K ,环戊烷温度为 296 K 和 235 K,环己烷温度为 294 K 和 222 K。这些光谱对于外星环境中的分子识别非常重要,例如土星的卫星泰坦、巨行星和系外行星。所有光谱均以数据点文件的形式提供。