Line-mixing effects in N2O Q branches:: Model, laboratory, and atmospheric spectra

被引:24
作者
Hartmann, JM
Bouanich, JP
Jucks, KW
Blanquet, G
Walrand, J
Bermejo, D
Domenech, JL
Lacome, N
机构
[1] Univ Paris Sud, Lab Phys Mol & Applicat, F-91405 Orsay, France
[2] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[3] Fac Univ Notre Dame Paix, Lab Spect Mol, B-5000 Namur, Belgium
[4] CSIC, Inst Estructura Mat, E-28006 Madrid, Spain
[5] Univ Paris 06, CNRS, UMR 7614, Lab Spect Mol, F-75252 Paris 05, France
[6] CNRS, UPR 1580, LADIR, F-94320 Thiais, France
关键词
D O I
10.1063/1.477862
中图分类号
O64 [物理化学(理论化学)、化学物理学];
学科分类号
070304 ; 081704 ;
摘要
A model based on the energy corrected sudden approximation is used in order to account for line-mixing effects in N2O Q branches of Sigma <-> Pi bands. The performance of this theoretical approach is demonstrated by comparisons with many (about 70) N2O-N-2 and N2O-O-2 laboratory spectra recorded in the 5 and 17 mu m regions by three instrument setups; the Q branches of the 2 nu(2)(0e) - nu(2)(1f) (near 579.3 cm(-1)), nu(2) (near 588.8 cm(-1)), and nu(2) + nu(3) (near 2798.3 cm(-1)) bands are investigated for different pressures (0.1-2.0 atm) and temperatures (200-300 K). The model is used to generate a set of line-mixing parameters for the calculation of the absorption by the nu(2) Q branch under atmospheric conditions. These data are tested by comparisons between computed stratospheric emissions and values measured using a balloon-borne high resolution Fourier transform instrument. The results confirm the need to account for the effects of line mixing and demonstrate the capability of the model to represent the N2O absorption in a region which can be used for the retrieval of N2O5 mixing ratios. (C) 1999 American Institute of Physics. [S0021-9606(99)01304-5].
引用
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页码:1959 / 1968
页数:10
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