15min:
BROADENING AND SHIFT COEFFICIENTS IN THE nu3 BANDS OF 12C16O2 AND 13C16O2.

M. A. H. SMITH, C. P. RINSLAND, Atmospheric Sciences, NASA Langley Research Center, Mail Stop 401A, Hampton, VA 23681-2199; D. CHRIS BENNER, V. MALATHY DEVI, Department of Physics, The College of William and Mary, Box 8795, Williamsburg, VA 23187-8795.

In a previous study we had reported N2-broadening and pressure-induced shift coefficients for 34 rovibrational transitions in the 12C16O2 nu3 fundamental band near 4.3 µm. These parameters were determined from spectra recorded with the McMath-Pierce Fourier transform spectrometer (FTS) of the National Solar Observatory on Kitt Peak, Arizona. We now report similar measurements of N2-broadening and shifts for transitions up to J''=56 in the 13C16O2 nu3 fundamental band, plus determinations of N2-broadening coefficients in the 13C16O2 nu2+ nu3- nu2 hot band and the 13C16O18O nu3 fundamental band. We also made new measurements of N2-broadening and pressure-induced shift coefficients for rovibrational transitions up to J''=46 in the 12C16O2 nu3 fundamental band. These results were obtained from simultaneous analysis of five absorption spectra using a multispectrum nonlinear least-squares technique. A 4.08 cm sample cell at room temperature was used to record all of the spectra at 0.003 cm-1 resolution with the McMath-Pierce FTS. This data set includes one low pressure (0.15 Torr) spectrum obtained with a 90% 13C-enriched CO2 sample and four spectra of lean mixtures of the same 13CO2 sample in N2. Total pressures of the mixtures were between 101 Torr and 464 Torr. Because of the isotopic sample used, the nu3 fundamental bands of 12CO2 and 13CO2 appeared together in the same spectra, and we were able to obtain a consistent set of line parameters for both molecules. The present measurements represent the first experimental determination of N2-broadening and pressure-induced shift coefficients in isotopic bands of CO2 in the 4.3 µm region. The results obtained for the various bands will be compared with each other, with the values in the HITRAN database, and with available values reported in the literature.