NH3 and PH3 line parameters:: the 2000 HITRAN update and new results

被引:59
作者
Kleiner, I
Tarrago, G
Cottaz, C
Sagui, L
Brown, LR
Poynter, RL
Pickett, HM
Chen, P
Pearson, JC
Sams, RL
Blake, GA
Matsuura, S
Nemtchinov, V
Varanasi, P
Fusina, L
Di Lonardo, G
机构
[1] Univ Paris 11, Photophys Mol Lab, F-91405 Orsay, France
[2] CNRS, F-75700 Paris, France
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Pacific NW Natl Lab, Richland, WA 99352 USA
[5] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[6] ISAS, Sagamihara, Kanagawa 2298510, Japan
[7] SUNY Stony Brook, Inst Terr & Planetary Atmospheres, Stony Brook, NY 11794 USA
[8] Dipartimento Chim Fis & Inorgan, I-40136 Bologna, Italy
基金
美国国家航空航天局;
关键词
ammonia; phosphine; molecular parameters; database;
D O I
10.1016/S0022-4073(03)00159-6
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
This paper describes the improvements incorporated into the 2000 version of the HITRAN database for ammonia (NH3), as well as newer results for phosphine (PH3) not included in HITRAN 2000. For ammonia the HITRAN 2000 database contains some 29084 ammonia lines, more than double the number of lines in HITRAN 1996. Specifically, the 2000 update involved replacing pure-rotational and infrared transitions from 0 to 3700 cm(-1) with new calculations for the (NH3)-N-14 isotopomer, whereas in the 4000 to 5300 cm(-1) region, parameters from the 1996 database were retained. The rotational quantum number range for line positions, intensities and line broadening parameters updated in this new HITRAN version goes up to J = 22, 15, 13 and 10 in the 8-1000 mum, 5 mum, 4 mum and 2.8-3.3 mum spectral regions respectively. For phosphine, a new database from 770 to 2156 cm(-1) available for future updates is described and contrasted with parameters in HITRAN 2000. (C) 2003 Elsevier Ltd. All rights reserved.
引用
收藏
页码:293 / 312
页数:20
相关论文
共 97 条
[1]  
Ainetschian A, 1996, J MOL SPECTROSC, V181, P99
[2]   Absorption intensities, pressure-broadening and line mixing parameters of some lines of NH3 in the ν4 band [J].
Aroui, H ;
Broquier, M ;
Picard-Bersellini, A ;
Bouanich, JP ;
Chevalier, M ;
Gherissi, S .
JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 1998, 60 (06) :1011-1023
[3]  
Atreya S. K., 1986, ATMOSPHERES IONOSPHE
[4]   A comparison of the atmospheres of Jupiter and Saturn: deep atmospheric composition, cloud structure, vertical mixing, and origin [J].
Atreya, SK ;
Wong, MH ;
Owen, TC ;
Mahaffy, PR ;
Niemann, HB ;
de Pater, I ;
Drossart, P ;
Encrenaz, T .
PLANETARY AND SPACE SCIENCE, 1999, 47 (10-11) :1243-1262
[5]   INVERSION AND INVERSION-ROTATION SPECTRUM OF (NH3)-N-14 IN THE NU-2 EXCITED-STATE [J].
BELOV, SP ;
GERSHSTEIN, LI ;
KRUPNOV, AF ;
MASLOVSKIJ, AV ;
URBAN, S ;
SPIRKO, V ;
PAPOUSEK, D .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1980, 84 (01) :288-304
[6]  
Belov SP, 1995, Z NATURFORSCH A, V50, P1187
[7]   Hyperfine structure of rotation-inversion levels in the excited ν2 state of ammonia [J].
Belov, SP ;
Urban, S ;
Winnewisser, G .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1998, 189 (01) :1-7
[8]   A NEW APPROACH TO THE TREATMENT OF ROTATIONAL SPECTRA OF MOLECULES WITH SMALL MOMENTS OF INERTIA APPLIED TO THE PH3 MOLECULE IN THE GROUND-STATE [J].
BELOV, SP ;
BURENIN, AV ;
POLYANSKY, OL ;
SHAPIN, SM .
JOURNAL OF MOLECULAR SPECTROSCOPY, 1981, 90 (02) :579-589
[9]  
BOUANICH JP, UNPUB JQSRT
[10]   A global high-resolution emission inventory for ammonia [J].
Bouwman, AF ;
Lee, DS ;
Asman, WAH ;
Dentener, FJ ;
VanderHoek, KW ;
Olivier, JGJ .
GLOBAL BIOGEOCHEMICAL CYCLES, 1997, 11 (04) :561-587