Spectral line parameters including temperature dependences of self- and air-broadening in the 2←0 band of CO at 2.3 μm

Abstract Temperature dependences of pressure-broadened half-width and pressure-induced shift coefficients along with accurate positions and intensities have been determined for transitions in the 2←0 band of 12C16O from analyzing high-resolution and high signal-to-noise spectra recorded with two different Fourier transform spectrometers. A total of 28 spectra, 16 self-broadened and 12 air-broadened, recorded using high-purity (≥99.5% 12C-enriched) CO samples and CO diluted with dry air (research grade) at different temperatures and pressures, were analyzed simultaneously to maximize the accuracy of the retrieved parameters. The sample temperatures ranged from 150 to 298 K and the total pressures varied between 5 and 700 Torr. A multispectrum nonlinear least squares spectrum fitting technique was used to adjust the rovibrational constants (G, B, D, etc.) and intensity parameters (including Herman–Wallis coefficients), rather than determining individual line positions and intensities. Self- and air-broadened Lorentz half-width coefficients, their temperature dependence exponents, self- and air-pressure-induced shift coefficients, their temperature dependences, self- and air- line mixing coefficients, their temperature dependences and speed dependence have been retrieved from the analysis. Speed-dependent line shapes with line mixing employing off-diagonal relaxation matrix element formalism were needed to minimize the fit residuals. This study presents a precise and complete set of spectral line parameters that consistently reproduce the spectrum of carbon monoxide over terrestrial atmospheric conditions.

[1]  Kendra L. Letchworth,et al.  RAPID AND ACCURATE CALCULATION OF THE VOIGT FUNCTION , 2007 .

[2]  Peter F. Bernath,et al.  The ACE-FTS atlas of the infrared solar spectrum , 2010 .

[3]  A. G. Maki,et al.  Absolute frequency measurements of the 2-0 band of CO at 2.3 μm; Calibration standard frequencies from high resolution color center laser spectroscopy , 1983 .

[4]  V. M. Devi,et al.  Cryogenic absorption cells operating inside a Bruker IFS-125HR: First results for 13CH4 at 7 μm , 2010 .

[5]  J. Bouanich,et al.  Pressure-Induced Lineshifts in the 2 ← 0 Band of CO Self-Perturbed and Perturbed by He, Kr, O2, and N2 , 1996 .

[6]  C. B. Farmer,et al.  Improved Dunham coefficients for CO from infrared solar lines of high rotational excitation , 1991 .

[7]  Prasad Varanasi,et al.  Measurement of line widths of CO of planetary interest at low temperatures , 1975 .

[8]  V. Malathy Devi,et al.  Line mixing and speed dependence in CO2 at 6348 cm-1: Positions, intensities, and air-and self-broadening derived with constrained multispectrum analysis , 2007 .

[9]  Prasad Varanasi,et al.  New laboratory data on the spectral line parameters in the 1-0 and 2-0 bands of relevant to atmospheric remote sensing , 2002 .

[10]  L. Brown,et al.  Self-broadened 12C16O line shapes in the v=2←0 band , 2003 .

[11]  Lawrence P. Giver,et al.  Absolute Rovibrational Intensities, Self-Broadening and Self-Shift Coefficients for the X(sup 1) Sigma(+) V=3 (left arrow) V=0 Band (C-12)(O-16) , 2001 .

[12]  Gang Li,et al.  The HITRAN 2008 molecular spectroscopic database , 2005 .

[13]  A. Weber,et al.  Spectroscopy of the Earth's Atmosphere and Interstellar Medium , 1992 .

[14]  P. Rosenkranz Shape of the 5 mm oxygen band in the atmosphere , 1975 .

[15]  J. Bouanich On the temperature dependence of self-broadening in the first overtone band of CO , 1984 .

[16]  V. M. Devi,et al.  A multispectrum nonlinear least squares fitting technique , 1995 .

[17]  T. A. Wiggins,et al.  Rotational and vibration constants of CO , 1965 .

[18]  Keeyoon Sung,et al.  Spectral line parameters including temperature dependences of air-broadening for the 2 ← 0 bands of 13C16O and 12C18O at 2.3 μm , 2012 .

[19]  T. Nakazawa,et al.  Intensities, half-widths and shapes of spectral lines in the fundamental band of CO at low temperatures. , 1982 .