Show simple item record

dc.creatorVaranasi, P.en_US
dc.creatorGiver, L. P.en_US
dc.creatorValero, Francisco P. J.en_US
dc.creatorGoorvitch, D.en_US
dc.date.accessioned2007-08-31T14:10:25Z
dc.date.available2007-08-31T14:10:25Z
dc.date.issued1982en_US
dc.identifier1982-FA-4en_US
dc.identifier.urihttp://hdl.handle.net/1811/29117
dc.description$^{\ast}$Supported in part by NASA Grant NGR 33-034-139.en_US
dc.description.abstractIn view of the recent observation of the $949 cm^{-1}$ fundamental band of ethylene in the atmospheres of Saturn and Titan made by the IRIS instrument on board the Voyager I spacecraft, we have studied this band as well as the $1443 cm^{-1}$ band at temperatures of 150K, 200K, and 296K, in the laboratory at NASA-Amea using a Nicolet interferometer-spectrometer and a cold cell developed at Stony Brook. Using nitrogen to broaden the rotational lines, the band strengths have been measured at 296K under conditions for which the rotational structure is smeared out. Using these results for the absolute intensities of the bands and the already published rotational analysis of these bands, we have made a comparison of a line-by-line calculation with our lower pressure spectra of the $C_{2}H_{4}$ nitrogen-broadened lines at temperatures of 150K, 200K, and 296K.en_US
dc.format.extent79433 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleA STUDY OF THE THERMAL INFRARED BANDS OF ETHYLENE AT LOW TEMPERATURESen_US
dc.typearticleen_US


Files in this item

Thumbnail

Items in Knowledge Bank are protected by copyright, with all rights reserved, unless otherwise indicated.

This item appears in the following Collection(s)

Show simple item record