共 50 条
Ammonia line lists from 1650 to 4000 cm-1
被引:24
|作者:
Hargreaves, Robert J.
[1
]
Li, Gang
[1
]
Bernath, Peter F.
[1
,2
]
机构:
[1] Univ York, Dept Chem, York YO10 5DD, N Yorkshire, England
[2] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA
关键词:
Emission spectra;
Molecules (ammonia);
Stars;
(cool;
low mass);
Brown dwarfs;
Atmospheric models;
Line lists;
INTERNAL PARTITION SUMS;
SPECTRAL TYPE-L;
ROVIBRATIONAL SPECTRA;
VIBRATIONAL SYSTEM;
INFRARED-SPECTRUM;
BROWN DWARFS;
(NH3)-N-14;
INTENSITIES;
NH3;
ASSIGNMENTS;
D O I:
10.1016/j.jqsrt.2012.02.033
中图分类号:
O43 [光学];
学科分类号:
070207 ;
0803 ;
摘要:
We present further line lists of ammonia (NH3) at high temperatures obtained by recording Fourier transform infrared emission spectra. Calibrated line lists are presented for 12 temperatures (300-1400 degrees C in 100 degrees C intervals) and each line list covers the 1650-4000 cm(-1) range, which includes the nu(1) and nu(3) fundamental modes (3 mu m) plus a number of combination, overtone and hot bands. Using our NH3 spectra, we have estimated empirical lower state energies (E-Low in cm(-1)) and our values have been incorporated into the line lists along with line positions ((nu) over bar in cm(-1)) and calibrated line intensities (S' in cm/molecule). We expect our hot NH3 line lists to find direct application in the modeling of planetary atmospheres and brown dwarfs. (C) 2012 Elsevier Ltd. All rights reserved.
引用
收藏
页码:670 / 679
页数:10
相关论文