CO2-broadened water in the pure rotation and m2 fundamental regions

The CO2-broadened water coefficients (half-widths, line shifts, and temperature dependence of the widths) are predicted using a fully complex Robert–Bonamy formulation for the 937 allowed and forbidden perpendicular type transitions of (000)–(000) between 200 and 900 cm!1 in order to facilitate atmospheric remote sensing of Mars and Venus. In addition, empirical Lorentz line widths and pressure-induced frequency-shifts of CO2-broadened H2 16O are obtained at room temperature for 257 perpendicular transitions of the (010)–(000) fundamental. For this, calibrated spectra recorded at 0.0054 cm!1 resolution are measured assuming Voigt line shapes. For transitions between 1287 and 1988 cm!1 with rotational quanta up to J = 13 and Ka = 6, the widths vary from 0.045 to 0.212 cm!1 atm!1 at 300 K; the pressure-shifts are quite large and range from!0.0386 to +0.0436 cm!1 atm!1. For the (010)–(000) band, the RMS and mean observed and calculated differences for CO2-broadened H2O half-widths are 12 % and!1.9%, respectively, while the RMS and mean ratios of the observed and calculated pressure-induced shift coefficients are 1.6 and 0.79, respectively. For pairs of transitions involving Ka = 0 and 1, such as 20 2 ‹ 313 and 313 ‹ 20 2, both the calculated and observed pressure induced shifts in positions are opposite in sign and often similar in magnitude. The data are too limited to characterize vibrational dependencies of the widths, however