Author:
Sromovsky L.A.,Fry P.M.,Boudon V.,Campargue A.,Nikitin A.
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference47 articles.
1. Global analysis of the high resolution infrared spectrum of methane 12CH4 in the region from 0 to 4800cm−1;Albert;Chem. Phys.,2009
2. The near-IR spectrum of Titan modeled with an improved methane line list;Bailey;Icarus,2011
3. The abundances of methane and ortho/para hydrogen on Uranus and Neptune: Implications of New Laboratory 4–0 H2 quadrupole line parameters;Baines;Icarus,1995
4. Boudon, V., Nikitin, T., Gabard, T., Wegner, C., Rey, M., Tyuterev, V.G., 2011. Theoretical modelling of the methane absorption spectrum for planetary applications. EPSC Abstracts, EPSC-DPS2011-115 6, 00.
5. Temperature dependence of the absorption spectrum of CH4 by high resolution spectroscopy at 81K: (II) The icosad region (1.49–1.30μm);Campargue;J. Quant. Spectrosc. Radiat. Trans.,2010
Cited by
66 articles.
订阅此论文施引文献
订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. First assignments of the 6ν4, ν2+5ν4, and ν1+4ν4 Triacontad band system of 12CH4 in the 7606-7919 cm−1 region;Journal of Quantitative Spectroscopy and Radiative Transfer;2024-10
2. Assignment and modeling of 13CH4 spectrum at 298 K in the lower part of the Tetradecad in the 4970–5300 cm−1 range;Journal of Quantitative Spectroscopy and Radiative Transfer;2024-09
3. Analysis of four solar occultations by Titan’s atmosphere with the infrared channel of the VIMS instrument: Haze, CH4, CH3D, and CO vertical profiles;Astronomy & Astrophysics;2022-10
4. Improved line list of 12CH4 in the 4100–4300 cm−1 region;Journal of Quantitative Spectroscopy and Radiative Transfer;2022-03
5. Line-strengths, collisional coefficients and narrowing parameters in the ν3 band of methane: H2, He, N2, O2, Ar and CO2 collider effects;Journal of Quantitative Spectroscopy and Radiative Transfer;2021-09