OCS-CO2 line broadening coefficients and their temperature dependences for the Earth and Venus atmospheres

Author:

Lavrentieva N.N.,Dudaryonok A.S.

Funder

Russian Science Foundation

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference27 articles.

1. Pressure broadening in the microwave and infra-red regions;Anderson;Phys.Rew.,1949

2. Spatially resolved measurements of H2O, HCl, CO, OCS, SO2, cloud opacity, and acid concentration in the Venus near-infrared spectral windows;Arney;J. Geophys. Res. Planets,2014

3. Fourier transform spectroscopy of carbonyl sulfide from 1800 to 3120 cm−1: the normal species;Belafhal;J. Mol. Spectrosc.,1995

4. Diode-laser measurements of Ar- and CO2-broadened linewidths in the v1 band of OCS;Bouanich;J. Quant. Spectrosc. Radiat. Trans.,1988

5. Influence of the collisional bending of trajectories on shifts of the molecular spectral lines in the visible region;Bykov;Atmosph. Ocean. Optics,1992

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2. H2, He, and CO2 Pressure-induced Parameters for the HITRAN Database. II. Line Lists of CO2, N2O, CO, SO2, OH, OCS, H2CO, HCN, PH3, H2S, and GeH4;The Astrophysical Journal Supplement Series;2022-09-22

3. КОЭФФИЦИЕНТЫ УШИРЕНИЯ И СДВИГА ЛИНИЙ OCS ДАВЛЕНИЕМ УГЛЕКИСЛОГО ГАЗА;XXVIII Международный симпозиум «Оптика атмосферы и океана. Физика атмосферы»;2022-06-22

4. The HITRAN2020 molecular spectroscopic database;Journal of Quantitative Spectroscopy and Radiative Transfer;2022-01

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