BROADENING AND SHIFTS OF $CH_{4}$ LINES IN THE $\nu_{4}$ BAND AT LOW TEMPERATURES

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1991

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Ohio State University

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We have recorded a series of high-resolution absorption spectra of methane broadened by dry air and by N2 at temperatures from −630C to 20C using the McMath Fourier transform spectrometer at the National Solar Observatory on Kitt Peak. The spectra cover a wavenumber range from approximately 500 cm−1 to 1500 cm−1 at a resolution of 0.01cm−1. These spectra have been analyzed to determine pressure broadening and line shift coefficients at low temperatures for over 150 lines in the ν4 fundamental band of 12CH4. These values, along with previous FTS measurements at room temperature1, have been used to determine the temperature dependence of the air- and N2-broadening and shift coefficients for these CH4 lines. Recent TDL measurements of low-temperature N2-broadening for a small group of lines2 are in excellent agreement with our results. Since the present results cover a wide range of rotational quantum numbers (J"" up to 13), the variation of the halfwidths and shift from line to line within the ν4 band will be examined.

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1C. P. Rinsland, V. Malathy Devi, M. A. H. Smith, and D. C. Benner, Appl. Opt. 27, 631-651 (1988). 2P. Varanasi and S. Chudamani, J. Geophys. Res 94, 13073-13078 (1989).""


Author Institution: Atmospheric Sciences Division, Mail Stop 401A, NASA Langley Research Center; Physics Department, College of William and Mary

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