Show simple item record

dc.creatorVaranasi, P.en_US
dc.creatorValero, Francisco P. J.en_US
dc.creatorGiver, L. P.en_US
dc.date.accessioned2007-08-31T14:10:30Z
dc.date.available2007-08-31T14:10:30Z
dc.date.issued1982en_US
dc.identifier1982-FA-7en_US
dc.identifier.urihttp://hdl.handle.net/1811/29120
dc.description$^{\ast}$Supported in part by NASA Grant NGR 33-034-139.en_US
dc.description.abstractThe 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.extent68501 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleINTENSITIES AND HALF-WIDTHS OF ACETYLENE LINES IN THE 3.04, 7.53, AND 13.7 MICRON BANDS 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