The rotational spectrum of HD broadened by H2 at temperatures between 100-296 K

被引:2
|
作者
Sung, Keeyoon [1 ]
Wishnow, Edward H. [2 ]
Drouin, Brian J. [1 ]
Manceron, Laurent [3 ]
Verseils, Marine [3 ]
Benner, D. Chris [4 ]
Nixon, Conor A. [5 ]
机构
[1] CALTECH, Jet Prop Lab, M-S 200-105, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[3] Synchrotron SOLEIL, AILES Beamline, F-91192 Gif Sur Yvette, France
[4] Coll William & Mary, Dept Phys, Williamsburg, VA 23187 USA
[5] NASA, Planetary Syst Lab, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
基金
美国国家航空航天局;
关键词
OUTER SOLAR-SYSTEM; INTRACOLLISIONAL INTERFERENCE; DIPOLE-MOMENT; LINE-SHAPES; COLLISIONAL INTERFERENCE; MONODEUTERATED METHANE; HITRAN DATABASE; QUADRUPOLE LINE; D/H RATIO; Q-BRANCH;
D O I
10.1016/j.jqsrt.2022.108412
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Laboratory measurements of the R(0) - R(3) pure rotational transitions of hydrogen deuteride (HD) have been performed at low pressures ( < 1 bar) and temperatures between 98 and 296 K. The measurements were conducted using a Fourier transform spectrometer coupled to the Soleil synchrotron far-infrared source to obtain pure HD and HD-H 2 mixture spectra. The observed spectra have been fitted using a non-linear least-squares multispectral fitting program. For each transition the line position, intensity, pressure broadening, pressure-induced frequency shift, and the temperature dependencies of these quantities have been determined simultaneously. These spectroscopic line parameters are compared to previous measurements made at higher gas pressures. Notably the present, and previous, measurements of the self-and H 2-broadened linewidths are smaller by a factor of five compared with those listed in the HITRAN and GEISA databases. This work is applicable to the low pressure, low temperature regimes found in the atmospheres of the giant gaseous planets. (C) 2022 Elsevier Ltd. All rights reserved.
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页数:14
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