The 1.28 μm transparency window of methane (7541–7919 cm−1): empirical line lists and temperature dependence (80 K–300 K)
The high sensitivity
The low energy values of the transitions observed at both room temperature and 80 K were derived from the variation of their line intensities. Empirical lower states and J values have been obtained for 2821 CH4 transitions representing 94.1 and 98.5% of the absorbance in the region at room temperature and 80 K, respectively. The good quality of these derived energy values is demonstrated by the marked propensity of the corresponding CH4 lower state J values to be close to integers. The constructed line lists extend to higher energies the WKC (Wang–Kassi–Campargue) line lists of methane in the near infrared (1.71–1.26 μm). They allow one accounting for the temperature dependence of methane absorption between 80 K and 300 K and are of importance for the analysis of the near infrared spectrum of several planetary bodies like Titan, Uranus and Neptune. The centers of the 3ν2 + ν3 and 6ν4 bands responsible of the absorption in the studied region are discussed in relation with recent theoretical calculations.