MEASUREMENTS OF $CH_{4} \\nu_{4}$ HALFWIDTHS USING TWO HIGH-RESOLUTION TECHNIQUES
V. Malathy Devi, Mary Ann H. Smith, CURTIS P. RINSLAND, D. Chris Benner
Abstract
V. Malathy Devi, Mary Ann H. Smith, CURTIS P. RINSLAND, D. Chris Benner
Abstract
Air-broadened and $N_{2}$-broadened halfwidths at room temperature for 25 lines in the $\\nu_{4}$ band of $^{12}CH_{4}$ have been determined from infrared absorption spectra recorded with a tunable diode laser (TDL) system in selected spectral regions between 1250 and $1360 cm^{-1}$. Air-broadened halfwidths for 20 of these lines were also determined from additional spectra at $0.01 cm^{-1}$ resolution recorded with the Fourier transform spectrometer (FTS) system in the McMath solar telescope complex on Kitt Peak. The air-broadened halfwidth values obtained from these two techniques are very consistent with agreement to better than 3% for most lines. Several additional lines of $^{13}CH_{4}$ and $^{12}CH_{3}D$ were also measured in the same spectral region with the diode laser system. The measured $N_{2}$-broadened and air-broadened halfwidths will be reported.
A significance statement is not available in the OpenAlex record.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
Air-broadened and $N_{2}$-broadened halfwidths at room temperature for 25 lines in the $\\nu_{4}$ band of $^{12}CH_{4}$ have been determined from infrared absorption spectra recorded with a tunable diode laser (TDL) system in selected spectral regions between 1250 and $1360 cm^{-1}$. Air-broadened halfwidths for 20 of these lines were also determined from additional spectra at $0.01 cm^{-1}$ resolution recorded with the Fourier transform spectrometer (FTS) system in the McMath solar telescope complex on Kitt Peak. The air-broadened halfwidth values obtained from these two techniques are very consistent with agreement to better than 3% for most lines. Several additional lines of $^{13}CH_{4}$ and $^{12}CH_{3}D$ were also measured in the same spectral region with the diode laser system. The measured $N_{2}$-broadened and air-broadened halfwidths will be reported.
Key concepts: Remote sensing, Geology