Empirical line parameters of methane in the 1.63-1.48 μm transparency window by high sensitivity Cavity Ring Down Spectroscopy

被引:40
作者
Campargue, A. [1 ]
Wang, L. [1 ]
Liu, A. W. [1 ,2 ]
Hu, S. M. [2 ]
Kassi, S. [1 ]
机构
[1] Univ Grenoble 1, Spectrometrie Phys Lab, CNRS, UMR 5588, F-384023 St Martin Dheres, France
[2] Univ Sci & Technol China, Hefei Natl Lab Phys Sci Microscale, Hefei 230026, Peoples R China
关键词
Methane; CH4; CH3D; Titan; CRDS; HITRAN; OUTER SOLAR-SYSTEM; MONODEUTERATED METHANE; TRANSITIONS; INTENSITIES; ABUNDANCE; VALUES; BAND; CH4;
D O I
10.1016/j.chemphys.2010.05.011
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070305 [高分子化学与物理];
摘要
The positions and intensities of methane in the 1.58 mu m transparency window have been measured by high sensitivity Cavity Ring Down Spectroscopy at room temperature. The achieved sensitivity allowed measuring intensities as small as 3 x 10(-29)cm/molecule i.e. three orders of magnitude smaller than the intensity cut off of the HITRAN line list of methane. The complete list contains a total of 16,149 transitions between 6165 and 6750 cm(-1). Their intensity values vary over six orders of magnitude from 1.6 x 10(-29) to 2.5 x 10(-23) cm/molecule. Transitions due to CH3D in "natural" abundance in our methane sample were identified using a new spectrum of CH3D recorded separately with a Fourier Transform spectrometer. From simulations of the CH3D and methane spectra at low resolution, the CH3D isotopologue has be found to contribute by up to 30% of the absorption near 1.58 mu m. (C) 2010 Elsevier B. V. All rights reserved.
引用
收藏
页码:203 / 210
页数:8
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