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

来源：

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2012年 / 113卷 / 09期

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

页码：670 / 679

页数：10

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