dc.creator Varanasi, P. en_US dc.creator Valero, Francisco P. J. en_US dc.creator Giver, L. P. en_US dc.date.accessioned 2007-08-31T14:10:30Z dc.date.available 2007-08-31T14:10:30Z dc.date.issued 1982 en_US dc.identifier 1982-FA-7 en_US dc.identifier.uri http://hdl.handle.net/1811/29120 dc.description $^{\ast}$Supported in part by NASA Grant NGR 33-034-139. en_US dc.description.abstract The absolute intensities of rotational lines of the acetylene bands at 3.04, 7.53, and 13.7 microns have been measured at temperatures of 150 K, 200 K, and 297 K. Hydrogen and nitrogen were used as broadening gases, and the pressure broadening determined for these gases at the different temperatures. The broadeners employed as well as the temperature range of the measurements make these spectra useful for interpretation of observations of the spectra of the major planets and Titan. The spectrum of the cooled gas in free of the hot banda'' observed at room temperature, simplifying the interpretation of the data. en_US dc.format.extent 68501 bytes dc.format.mimetype image/jpeg dc.language.iso English en_US dc.publisher Ohio State University en_US dc.title INTENSITIES AND HALF-WIDTHS OF ACETYLENE LINES IN THE 3.04, 7.53, AND 13.7 MICRON BANDS AT LOW TEMPERATURES en_US dc.type article en_US
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