{"title":"Water vapor line broadening and shift coefficients induced by carbon dioxide in the 8600–9000 cm-1 spectral region","authors":"T.M. Petrova, A.M. Solodov, A.A. Solodov, V.M. Deichuli, N.N. Lavrentieva, A.S. Dudaryonok","doi":"10.1016/j.jqsrt.2025.109577","DOIUrl":null,"url":null,"abstract":"<div><div>Water vapor line broadening and shift coefficients induced by carbon dioxide are important for different problems of atmospheric physics, astrophysics, and laser physics. The database HITRAN contains the mentioned parameters for non-Earth atmospheres such as Mars and Venus, but it is not complete. Measured and computed line-broadening and shift coefficients for R-, P- and Q-branches in the ν<sub>1</sub>+ν<sub>2</sub>+ν<sub>3</sub> band in comparison with data in the ν<sub>2</sub>+ν<sub>3</sub> band are presented. New absorption spectra were recorded using a Bruker IFS 125 HR FTIR spectrometer, a multispectrum fitting procedure was applied to recover the spectral line parameters using the speed-dependent Voigt profile. Line parameters of H<sub>2</sub>O<img>CO<sub>2</sub> were computed by a semi-empirical method for rotational quantum numbers <em>J</em> from 0 till 20. The vibrational dependence of obtained data is discussed.</div></div>","PeriodicalId":16935,"journal":{"name":"Journal of Quantitative Spectroscopy & Radiative Transfer","volume":"345 ","pages":"Article 109577"},"PeriodicalIF":1.9000,"publicationDate":"2025-07-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Quantitative Spectroscopy & Radiative Transfer","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0022407325002390","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"OPTICS","Score":null,"Total":0}
引用次数: 0
Abstract
Water vapor line broadening and shift coefficients induced by carbon dioxide are important for different problems of atmospheric physics, astrophysics, and laser physics. The database HITRAN contains the mentioned parameters for non-Earth atmospheres such as Mars and Venus, but it is not complete. Measured and computed line-broadening and shift coefficients for R-, P- and Q-branches in the ν1+ν2+ν3 band in comparison with data in the ν2+ν3 band are presented. New absorption spectra were recorded using a Bruker IFS 125 HR FTIR spectrometer, a multispectrum fitting procedure was applied to recover the spectral line parameters using the speed-dependent Voigt profile. Line parameters of H2OCO2 were computed by a semi-empirical method for rotational quantum numbers J from 0 till 20. The vibrational dependence of obtained data is discussed.
期刊介绍:
Papers with the following subject areas are suitable for publication in the Journal of Quantitative Spectroscopy and Radiative Transfer:
- Theoretical and experimental aspects of the spectra of atoms, molecules, ions, and plasmas.
- Spectral lineshape studies including models and computational algorithms.
- Atmospheric spectroscopy.
- Theoretical and experimental aspects of light scattering.
- Application of light scattering in particle characterization and remote sensing.
- Application of light scattering in biological sciences and medicine.
- Radiative transfer in absorbing, emitting, and scattering media.
- Radiative transfer in stochastic media.