An improved empirical line list for methane in the region of the 2ν3 band at 1.66 μm

被引:31
作者
Campargue, A. [1 ]
Leshchishina, O. [1 ]
Mondelain, D. [1 ]
Kassi, S. [1 ]
Coustenis, A. [2 ]
机构
[1] Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France
[2] Univ Paris 07, Observ Paris, CNRS, Lab Etudes Spatiales & Instrumentat Astrophys,UMR, F-92195 Meudon, France
关键词
Methane; CH4; Near infrared; Absorption spectroscopy; HITRAN; GOSAT; M TRANSPARENCY WINDOW; TEMPERATURE-DEPENDENCE; CAVITY RING; CM(-1); SPECTROSCOPY; TRANSITIONS; VALUES; STATE;
D O I
10.1016/j.jqsrt.2012.12.004
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The absorption spectrum of methane is recorded at room temperature by differential absorption spectroscopy (DAS) in the high energy part of the tetradecad (5855-6183 cm(-1)) dominated by the 2 nu(3) band at 1.66 mu m. An empirical list of 9228 lines is constructed from a profile fitting of the very congested spectrum. The achieved noise equivalent absorption of the spectra (alpha(min) approximate to 1 x 10(-7) cm(-1)) allowed us to add about 4000 lines to the recent empirical list constructed in relation with the project "Green-house Gases Observing Satellite" (Nikitin A, Lyulin O, Mikhailenko S, Perevalov V, Filippov N, Grigoriev I, et al. GOSAT-2009 methane spectral list in the 5550-6236 cm(-1) range. J Quant Spectrosc Radiat Transfer 2010;111:2211-24). Lines due to the (CH4)-C-13 and CH3D isotopologues present in the methane sample in "natural" abundance (0.011 and 5.0 x 10(-4), respectively) are systematically identified by comparison with spectra of pure CH3D and (CH4)-C-13 recorded separately. In order to derive empirical values of the lower state energy level, E-emp, from the intensity ratios of the lines measured at 80 K and 296 K, the obtained 296 K line list is combined with the WKMC list of methane at 80 K (Campargue A, Leshchishina O, Wang L, Mondelain D, Kassi S, Nikitin AV. Refinements of the WKMC empirical line lists (5852-7919 cm(-1)) for methane between 80 K and 296 K. J Quant Spectrosc Radiat Transfer 2012;113:1855-73). Overall 4396 lower state energy values were determined extending significantly the previous set of Eemp values derived using the GOSAT list for the room temperature dataset. These improvements allow for a better accounting of the methane spectrum temperature dependence between 80 K and 300 K. A number of discrepancies between the rovibrational assignments included in the GOSAT list and our derived E-emp values is discussed. The new line dataset including a large number of empirical lower state energies provides a solid basis for future theoretical modeling of the tetradecad of (CH4)-C-12. (c) 2012 Elsevier Ltd. All rights reserved.
引用
收藏
页码:49 / 59
页数:11
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