The CW-Cavity Ring Down Spectrum of CH4 has been recorded in the 1.55 µm transparency window with a very high sensitivity
Résumé
The high resolution absorption spectrum of methane has been recorded at room temperature by high sensitivity CW-Cavity Ring Down Spectroscopy between 1.50 and 1.60 m (6250-6680 cm-1). This spectral region has a low opacity and is then of particular interest for the spectral analysis of the outer planets and Titan. The recordings were performed with a sensitivity corresponding to a noise equivalent absorption of min~510-10 cm-1 and allowed for the detection of lines with an intensity smaller than 10-28 cm/molecule far beyond the weakest lines provided by the HITRAN database. The spectrum exhibits a highly complex and congested structure with a kind of “fractal” character and a density of transitions of a few tens per cm-1. The impact of the weak newly observed transitions on the total absorption in the region is discussed.
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