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dc.creatorHansen, Peteren_US
dc.creatorStrong, Johnen_US
dc.date.accessioned2006-06-15T13:32:55Z
dc.date.available2006-06-15T13:32:55Z
dc.date.issued1972en_US
dc.identifier1972-O-7en_US
dc.identifier.urihttp://hdl.handle.net/1811/9079
dc.descriptionAuthor Institution: Astronomy Research Facility, University of Massachusettsen_US
dc.description.abstractWater vapor absorption lines from 1400 to $1700 cm^{-1}$ are studied at $0.07 cm^{-1}$ resolving power, using our Hadamard Transform Spectrometer (Appl. Opt. 11, March 1972). This includes the lines reported by Fridovich and Kinard last year. The absorption path conditions are the same -- 92 -- meter geometrical path through pure water vapor at p $<$ 10 mm Hg. The isolated absorption lines are interpreted by curves of growth; the central peak absorption; and maximum slopes, $dA/d\nu$. The purpose of this investigation is to check $S\cdot \gamma$ values in the literature against observations as they apply to conditions near those that obtain in the interstellar medium.en_US
dc.format.extent92427 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titlePURE WATER VAPOR ABSORPTION MEASUREMENTS IN 6.3 MICRON BANDen_US
dc.typearticleen_US


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