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dc.creatorFox, K.en_US
dc.creatorMargolis, J. S.en_US
dc.date.accessioned2006-06-15T16:50:05Z
dc.date.available2006-06-15T16:50:05Z
dc.date.issued1969en_US
dc.identifier1969-E-3en_US
dc.identifier.urihttp://hdl.handle.net/1811/15691
dc.descriptionKenneth Fox has been an NRC-NASA Resident Research Associate, on leave from the Department of Physics and Astronomy, The University of Tennessee (address for academic year 1969-70). J.S. Margolis acknowledges support by NASA Contract NAS 7-100. $^{1}$ J.S. Margolis and Kenneth Fox, J. Chem. Phys. 49, 2451 (1968).en_US
dc.descriptionAuthor Institution: Jet Propulsion Laboratory, California Institue of Technologyen_US
dc.description.abstractHigh resolution laboratory $measurements^{1}$ of line positions and relative intensities of fine structure components in the methane band at 9050 $cm^{-1}$, as well as new theoretical results, have been used to deduce properties of the Jovian atmosphere. Saturation was found to be important for a large range of Lorentz half-widths $\gamma$. Results are presented for $0.03\leq \gamma \leq 0.30 cm^{-1}$ and for no saturation.en_US
dc.format.extent112096 bytes
dc.format.mimetypeimage/jpeg
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleHIGH RESOLUTION TECHNIQUES FOR METHANE IN THE JOVIAN ATMOSPHERE.en_US
dc.typearticleen_US


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