NEAR INFRARED SPECTROSCOPY OF CARBON DIOXIDE: $^{16}O^{12}C^{16}O$ LINE POSITIONS

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2003

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Ohio State University

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High-resolution near infrared 4000−9000cm−1 spectra of carbon dioxide have been recorded using the McMath-Pierce Fourier transform spectrometer at the Kitt Peak National Solar Observatory. Spectroscopic constants have been determined for 53 different vibrational states of the 16O12C16O isotopologue, including 8 vibrational states for which laboratory spectra have not previously been reported. Calibration using the 2-0 band of CO near 4200cm−1 and the (ν1+ν3) combination band of C2H2 near 6500cm−1 provides absolute line position accuracies of 2×10−5cm−1 (RMS) for strong, isolated transitions throughout the observed range. Fits with RMS errors less than 3.8×10−5cm−1 have been obtained for the 20013←00001,20012←00001, and 20011←00001 bands and RMS errors less than 6×10−5cm−1 have been obtained for the 30014←00001,30013←00001,30012←00001, and 00031←00001 bands. The new line list satisfies the line position accuracies required for the next generation of CO2 remote sensing instruments, improves the capability of solarviewing spectrometers to retrieve precise column CO2 measurements, and provides a secondary frequency standard in the NIR.a

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aPart of the research described in this paper was carried out by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.


Author Institution: Department of Chemistry, Haverford College; Jet Propulsion Laboratory, California Institute of Technology

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