Absorption cross sections of n-butane, n-pentane, cyclopentane and cyclohexane

被引：2

作者：

Sorensen, Jason J. ^{[1
]}

Bernath, Peter F. ^{[1
,2
]}

Johnson, Ryan M. ^{[2
]}

Dodangodage, Randika ^{[2
]}

Cameron, W. Doug ^{[2
]}

LaBelle, Keith ^{[2
]}

机构：

[1] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA

[2] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2022年 / 290卷

关键词：

Infrared spectroscopy; Absorption cross sections; Planetary atmospheres; Fourier transform spectroscopy; Hydrocarbons; VIBRATIONAL-SPECTRA; INFRARED-SPECTRUM; ORGANIC HAZE; FORCE-FIELD; RAMAN; ATMOSPHERE; ETHANE; PHOTOCHEMISTRY; STRATOSPHERE; INTENSITIES;

D O I：

10.1016/j.jqsrt.2022.108284

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

The infrared absorption cross sections of pure n-butane, n-pentane, cyclopentane and cyclohexane have been measured in the 3.3 mu m region (and 6.8 mu m 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. (C) 2022 Elsevier Ltd. All rights reserved.

引用

页数：5

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