A methane line list with sub-MHz accuracy in the 1250 to 1380 cm-1 range from optical frequency comb Fourier transform spectroscopy
arXiv:2204.06356 · doi:10.1016/j.jqsrt.2022.108252
Abstract
We use a Fourier transform spectrometer based on a difference frequency generation optical frequency comb to measure high-resolution, low-pressure, room-temperature spectra of methane in the 1250 - 1380 cm range. From these spectra, we retrieve line positions and intensities of 678 lines of two isotopologues: 157 lines from the CH fundamental band, 131 lines from the CH fundamental band, as well as 390 lines from two CH hot bands, + - and 2 - . For another 165 lines from the CH fundamental band we retrieve line positions only. The uncertainties of the line positions range from 0.19 to 2.3 MHz, and their median value is reduced by a factor of 18 and 59 compared to the previously available data for the CH fundamental and hot bands, respectively, obtained from conventional FTIR absorption measurements. The new line positions are included in the global models of the spectrum of both methane isotopologues, and the fit residuals are reduced by a factor of 8 compared to previous absorption data, and 20 compared to emission data. The experimental line intensities have relative uncertainties in the range of 1.5 - 7.7%, similar to those in the previously available data; 235 new CH line intensities are included in the global model.
References in corpus (12)
- Water, Methane, and Carbon Dioxide Present in the Dayside Spectrum of the Exoplanet HD 209458b
- A ground-based near-infrared emission spectrum of the exoplanet HD 189733b
- Surpassing the Path-Limited Resolution of a Fourier Transform Spectrometer with Frequency Combs
- Probing the terminator region atmosphere of the Hot-Jupiter XO-1b with transmission spectroscopy
- Optical Frequency Comb Fourier Transform Spectroscopy with Sub-Nominal Resolution - Principles and Implementation
- Quantum state resolution of the C fullerene
- Detection of CO in Triton's atmosphere and the nature of surface-atmosphere interactions
- Methane depletion in both polar regions of Uranus inferred from HST/STIS and Keck/NIRC2 observations
- High-resolution and gapless dual comb spectroscopy with current-tuned quantum cascade lasers
- A mid-infrared dual-comb spectrometer in step-sweep mode for high-resolution molecular spectroscopy
- Sub-Doppler Double-Resonance Spectroscopy of Methane Using a Frequency Comb Probe
- Optical Frequency Comb Fourier Transform Spectroscopy of NO at 7.8 μm