Spectroscopic characterization of the v2=3 and v2 = v4=1 states for 15NH3 from high resolution infrared spectra

被引:4
|
作者
Cane, Elisabetta [1 ]
Di Lonardo, Gianfranco [1 ]
Fusina, Luciano [1 ]
Tamassia, Filippo [1 ]
Predoi-Cross, Adriana [2 ]
机构
[1] Univ Bologna, Dipartimento Chim Ind Toso Montanari, Viale Risorgimento 4, I-40136 Bologna, Italy
[2] Univ Lethbridge, Alberta Terr Imaging Ctr, Dept Phys & Astron, 4401 Univ Dr, Lethbridge, AB T1K 3M4, Canada
基金
加拿大自然科学与工程研究理事会; 加拿大健康研究院; 加拿大创新基金会;
关键词
Ammonia; (NH3)-N-15; High resolution infrared spectrum; Vibration-excited bending states; NITROGEN; AMMONIA; ORIGIN; INTENSITIES; DEPOSITION; EMISSIONS; JUPITER; SYSTEM; COMETS;
D O I
10.1016/j.jqsrt.2020.106987
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The a, s inversion levels of v(2) = 3 and v(2) = v(4) = 1 vibration states of (NH3)-N-15 are studied from high resolution infrared spectra up to 3200 cm(-1). Spectra were recorded from 60 to 2000 cm(-1) using the Bruker IFS 125 interferometer located at the Canadian Light Source and from 1900 to 3200 cm(-1) using the Bomem DA 008 in Bologna. Transitions in 3v(2) and v(2) + v(4) , in the 3v(2) <- v(2), v(2) + v(4) <- v(2), 3v(2) <- 2v(2), v(2) + v(4) <- 2v(2), 3v(2) <- v(4), v(2) + v(4) <- v(4), and 3v(2) <-> v(2) + v(4) hot bands, and the rotation-inversion transitions in 3v(2) and v(2) + v(4) have been observed. 5770 transitions with J'(max)/K'(max) up to 15 have been assigned, including 395 perturbation allowed ones. All transitions were fitted simultaneously on the basis of a rotation-inversion Hamiltonian which includes distortion constants up to 10th power in the angular momentum and all symmetry allowed interaction parameters between and within the a, s inversion levels of v(2) = 3 and v(2) = v(4) = 1. The term values of the lower levels of transitions have been calculated using the parameters recently derived for the ground and v(2) = 1, 2 and v(4) = 1 states. The data were reproduced at experimental accuracy. The results are compared with those of (NH3)-N-14. The experimental transitions are compared with their theoretically predicted values. The list of assignments is supplied as supplementary material. The present results noticeably improve the wavenumber line list in the HITRAN 2016 data base. (C) 2020 Elsevier Ltd. All rights reserved.
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