15min:
MEASUREMENTS OF AIR-BROADENING AND PRESSURE-SHIFT COEFFICIENTS AND LINE MIXING IN THE nu6 FUNDAMENTAL BAND OF 12CH3D.

V. MALATHY DEVI, D. CHRIS BENNER, Department of Physics, The College of William and Mary, Box 8795, Williamsburg, VA 23187-8795; MARY ANN H. SMITH, CURTIS P. RINSLAND, Atmospheric Sciences, NASA Langley Research Center, Mail Stop 401A, Hampton, VA 23681-2199; AND LINDA R. BROWN, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109.

A multispectrum nonlinear least-squares spectral fitting technique has been used to measure air-broadening and air induced pressure-shift coefficients for more than 670 transitions in the nu6 fundamental band of 12CH3D in the 1040 and 1410 cm-1 spectral region. Additionally, line mixing effects were observed and values for off diagonal relaxation matrix coefficients were determined for the first time in several of the K''=3, A+A- split components in the PP, PQ, PR, RP, RQ, and RR sub-band transitions. These results were obtained from simultaneous analysis of 11 room temperature laboratory absorption spectra recorded with the McMath-Pierce Fourier transform spectrometer at the National Solar Observatory on Kitt Peak, Arizona. Low-pressure (1 to 3 torr) spectra of 98% pure CH3D and lean mixtures (~ 1%) of CH3D in dry air (100 to 400 torr) in 25 and 150 cm pathlength absorption cells were used in the analysis. Measurements involved transitions with quantum numbers as high as J''=17 and K''=15 and also included 34 transitions with 2 \leq Delta K \leq 4. The air-broadening coefficients range between 0.016 and 0.076 cm-1 atm-1 at 296K and the pressure-shift coefficients vary from about -0.012 to +0.008 cm-1 atm-1. For each J series in the PP and RR sub-bands, the J''=K'' (or the J'=K') transition exhibited the smallest broadening coefficient. In the PQ sub-band, J''=K'' transition in each J series had the largest negative pressure-shift coefficient while the J'=K' transition lines in the RQ sub-band showed the largest positive pressure-shift coefficients. These and several other interesting patterns observed during the analysis will be discussed. The results will be compared to previous measurements and to other values reported in the literature.