2003
DOI: 10.1016/s0022-4073(03)00155-9
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Methane line parameters in HITRAN

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Cited by 125 publications
(71 citation statements)
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“…This is possibly caused by the more poorly understood spectroscopy of methane, specifically the lack of accurate air-broadening coefficients and temperature dependencies, which has been noted by Rothman et al (2005), Brown et al (2003) and Worden et al (2004).…”
Section: Resultsmentioning
confidence: 99%
“…This is possibly caused by the more poorly understood spectroscopy of methane, specifically the lack of accurate air-broadening coefficients and temperature dependencies, which has been noted by Rothman et al (2005), Brown et al (2003) and Worden et al (2004).…”
Section: Resultsmentioning
confidence: 99%
“…[140,141]. For the pentad, about 500 prior measurements [138] were used along with approximately 3800 predicted values for γ air , n, and δ of the ν 3 transitions from Antony et al [142]. Scaled N 2 -broadening from Frankenberg et al [132] were inserted from 5860 to 6184 cm -1 and a few hundred values for γ air , were entered between 5560 to 5860 cm -1 [143].…”
Section: Ch 4 (Molecule 6)mentioning
confidence: 99%
“…Since Raman and Rayleigh scattering contributions are limited, this spectral region presents significant advantages for reliable quantitative interpretation of theoretical and/or observational atmospheric and astrophysical data. Methane (CH 4 ), which is an important atmospheric constituent in many planetary systems, has dense transition lines with strong absorption near 3-4 µm [1][2]. Identification and quantification of these lines in the spectrum are of considerable interest for the retrieval of CH 4 abundance in planetary atmosphere.…”
Section: Introductionmentioning
confidence: 99%