HIGH RESOLUTION TECHNIQUES FOR METHANE IN THE JOVIAN ATMOSPHERE.

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Title: HIGH RESOLUTION TECHNIQUES FOR METHANE IN THE JOVIAN ATMOSPHERE.
Creators: Fox, K.; Margolis, J. S.
Issue Date: 1969
Publisher: Ohio State University
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.
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).
Author Institution: Jet Propulsion Laboratory, California Institue of Technology
URI: http://hdl.handle.net/1811/15691
Other Identifiers: 1969-E-3
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