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dc.creatorNiple, E.en_US
dc.creatorMankin, W. G.en_US
dc.creatorGoldman, A.en_US
dc.creatorMurcray, D. G.en_US
dc.date.accessioned2006-06-15T14:33:50Z
dc.date.available2006-06-15T14:33:50Z
dc.date.issued1980en_US
dc.identifier1980-TA-13en_US
dc.identifier.urihttp://hdl.handle.net/1811/11330
dc.description$^{1}$Y. S. Chang And J. H. Shaw, Appl. Spectrosc., 31, 213 (1977).en_US
dc.descriptionAuthor Institution:en_US
dc.description.abstractNonlinear least squares spectral curve $fitting^{1}$ has been used to analyze a narrow spectral region (1603 – $1607.4 cm^{-1}$) from a series of solar occulation spectra collected with a high resolution (=$0.02 cm^{-1}$) interferometer. These spectra were used to retrieve the vertical mixing ratio profiles for $NO_{2}$ and $H_{2}O$ above 16 km. After standard phase correction and removal of the secondary interferogram, some residual phase error and channel spectrum distortion remained and interfered with the profile retrievals. By explicitly including both these effects in the spectral model and simultaneously retrieving the phase error and channel spectrum parameters a long with the other parameters (background level, instrument resolution, frequency shift, $NO_{2}$ and $H_{2}O$ profiles and relevant temperatures) improved profiles were obtained.en_US
dc.format.extent98039 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleANALYSIS OF HIGH RESOLUTION SPECTRA IN THE PRESENCE OF CHANNEL SPECTRA AND PHASE ERRORS USING NONLINEAR LEAST SQUARESen_US
dc.typearticleen_US


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