共 30 条
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.
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Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France

Leshchishina, O.
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Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France

Mondelain, D.
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Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France

Kassi, S.
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Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France

Coustenis, A.
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Univ Paris 07, Observ Paris, CNRS, Lab Etudes Spatiales & Instrumentat Astrophys,UMR, F-92195 Meudon, France Univ Grenoble 1, CNRS, UMR5588, LIPhy, F-38041 Grenoble, France
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.
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页码:49 / 59
页数:11
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Kassi, Samir
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Univ Grenoble 1, UMR CNRS 5588, Lab Interdisciplinaire Phys LIPhy, F-38402 St Martin Dheres, France Univ Paris 07, Observ Paris, UMR CNRS 8109, LESIA, F-92195 Meudon, France

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Univ Grenoble 1, UMR CNRS 5588, Lab Interdisciplinaire Phys LIPhy, F-38402 St Martin Dheres, France Univ Paris 07, Observ Paris, UMR CNRS 8109, LESIA, F-92195 Meudon, France

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Russian Acad Sci, Inst Atmospher Opt, Lab Theoret Spect, Tomsk 634055, Russia Univ Paris 07, Observ Paris, UMR CNRS 8109, LESIA, F-92195 Meudon, France

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Univ Oxford, Dept Phys, Clarendon Lab, Oxford OX1 3PU, England Univ Oxford, Dept Phys, Clarendon Lab, Oxford OX1 3PU, England

Hurley, J.
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Univ Oxford, Dept Phys, Clarendon Lab, Oxford OX1 3PU, England Univ Oxford, Dept Phys, Clarendon Lab, Oxford OX1 3PU, England
[10]
The near-infrared (1.30-1.70 μm) absorption spectrum of methane down to 77 K
[J].
Kassi, Samir
;
Gao, Bo
;
Romanini, Daniele
;
Campargue, Alain
.
PHYSICAL CHEMISTRY CHEMICAL PHYSICS,
2008, 10 (30)
:4410-4419

Kassi, Samir
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Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France

Gao, Bo
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Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France
Univ Sci & Technol China, Dept Chem Phys, Hefei Natl Lab Phys Sci Microscale, Hefei 230026, Peoples R China Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France

Romanini, Daniele
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Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France

Campargue, Alain
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Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France Univ Grenoble 1, CNRS, Spectrometrie Phys Lab, UMR 5588, F-38402 St Martin Dheres, France