The 13CH4 absorption spectrum in the Icosad range (6600-7692 cm-1) at 80 K and 296 K: Empirical line lists and temperature dependence

被引:17
作者
Campargue, A. [1 ,2 ]
Beguier, S. [1 ,2 ]
Zbiri, Y. [1 ,2 ]
Mondelain, D. [1 ,2 ]
Kassi, S. [1 ,2 ]
Karlovets, E. V. [3 ]
Nikitin, A. V. [3 ,4 ]
Rey, M. [5 ]
Starikova, E. N. [3 ,4 ]
Tyuterev, Vl G. [5 ]
机构
[1] Univ Grenoble Alpes, LIPhy, F-38000 Grenoble, France
[2] CNRS, LIPhy, F-38000 Grenoble, France
[3] Tomsk State Univ, Lab Quantum Mech Mol & Radiat Proc, 36 Lenin Ave, Tomsk 634050, Russia
[4] IAO SB RAN, Lab Theoret Spect, Av 1,Akademician Zuev Sq, Tomsk 634021, Russia
[5] Univ Reims, UMR CNRS 7331, GSMA, Moulin Housse,BP 1039, F-51687 Reims 2, France
关键词
Methane; (CH4)-C-13; Isotope; Absorption spectroscopy; HITRAN; M TRANSPARENCY WINDOW; 1.66; MU-M; 2-NU(3) BAND; METHANE; REGION; SPECTROSCOPY; TRANSITIONS; PARAMETERS; VALUES;
D O I
10.1016/j.jms.2016.01.005
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
The (CH4)-C-13 absorption spectrum has been recorded at 296 K and 80 K in the Icosad range between 6600 and 7700 cm(-1). The achieved noise equivalent absorption of the spectra recorded by differential absorption spectroscopy (DAS) is about alpha(min) approximate to 1.5 x 10(-7) cm(-1). Two empirical line lists were constructed including 17,792 and 24,139 lines at 80 K and 296 K, respectively. For comparison, the HITRAN database provides only 1040 (CH4)-C-13 lines in the region determined from methane spectra with natural isotopic abundance. Empirical values of the lower state energy level, E-emp, were systematically derived from the intensity ratios of the lines measured at 80 K and 296 K. Overall 10,792 E-emp values were determined providing accurate temperature dependence for most of the (CH4)-C-13 absorption in the region (93% and 82% at 80 K and 296 K, respectively). The quality of the derived empirical values of the lower state rotational quantum number, J(emp), is illustrated by their clear propensity to be close to an integer. A good agreement is achieved between our small J(emp), values, with previous accurate determinations obtained by applying the 2T method to jet and 80 K spectra. The line lists at 296 K and 80 K which are provided as Supplementary material will be used for future rovibrational assignments based on accurate variational calculations. (C) 2016 Elsevier Inc. All rights reserved.
引用
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页码:115 / 121
页数:7
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