Improvement of the spectroscopic parameters of the air- and self-broadened N2O and CO lines for the HITRAN2020 database applications

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作者
Hashemi, Robab [1 ]
Gordon, Iouli E. [1 ]
Adkins, Erin M. [2 ]
Hodges, Joseph T. [2 ]
Long, David A. [2 ]
Birk, Manfred [3 ]
Loos, Joep [3 ]
Boone, Chris D. [4 ]
Fleisher, Adam J. [2 ]
Predoi-Cross, Adriana [5 ]
Rothman, Laurence S. [1 ]
机构
[1] Atomic and Molecular Physics Division, Harvard-Smithsonian Center for Astrophysics, Cambridge,MA, United States
[2] National Institute of Standards and Technology, Gaithersburg,MD,20899, United States
[3] Remote Sensing Technology Institute, German Aerospace Center (DLR), Wessling,D-82234, Germany
[4] Department of Chemistry, University of Waterloo, Ontario, Canada
[5] Independent Researcher, Lethbridge,AB, Canada
基金
美国国家航空航天局;
关键词
Database systems - Temperature distribution - Mixing - Molecules - Nitrogen oxides;
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摘要
This paper outlines the major updates of the line-shape parameters that were performed for the nitrous oxide (N2O) and carbon monoxide (CO) molecules listed in the HITRAN2020 database. We reviewed the collected measurements for the air- and self-broadened N2O and CO spectra to determine proper values for the spectroscopic parameters. Careful comparisons of broadening parameters using the Voigt and speed-dependent Voigt line-shape profiles were performed among various published results for both N2O and CO. Selected data allowed for developing semi-empirical models, which were used to extrapolate/interpolate existing data to update broadening parameters of all the lines of these molecules in the HITRAN database. In addition to the line broadening parameters (and their temperature dependences), the pressure shift values were revised for N2O and CO broadened by air and self for all the bands. The air and self speed-dependence of the broadening parameter for these two molecules were added for every transition as well. Furthermore, we determined the first-order line-mixing parameters using the Exponential Power Gap (EPG) scaling law. These new parameters are now available at HITRANonline. © 2021 Elsevier Ltd
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