dc.creator Fox, K. en_US dc.creator Margolis, J. S. en_US dc.date.accessioned 2006-06-15T16:50:05Z dc.date.available 2006-06-15T16:50:05Z dc.date.issued 1969 en_US dc.identifier 1969-E-3 en_US dc.identifier.uri http://hdl.handle.net/1811/15691 dc.description Kenneth 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.description Author Institution: Jet Propulsion Laboratory, California Institue of Technology en_US dc.description.abstract High 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.extent 112096 bytes dc.format.mimetype image/jpeg dc.language.iso English en_US dc.publisher Ohio State University en_US dc.title HIGH RESOLUTION TECHNIQUES FOR METHANE IN THE JOVIAN ATMOSPHERE. en_US dc.type article en_US
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