Computer Science
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982vrsp....2..549l&link_type=abstract
In NASA. Goddard Space Flight Center Vibrational-Rotational Spectry. for Planetary Atmospheres, Vol. 2 p 549-555 (SEE N82-2613
Computer Science
Atmospheric Composition, Hydrogen, Methane, Neptune Atmosphere, Uranus Atmosphere, Line Spectra, Molecular Spectroscopy, Pressure Broadening, Quadrupoles, Spectroscopic Analysis
Scientific paper
A feature near 6420 A which appears in the spectra of Uranus and Neptune, and was recently detected in the spectrum of Titan is investigated. When originally identified, it was assigned to the pressure induced 4 to 0 band of molecular hydrogen. Not only did the wavelength agree--a small apparent shift was arm waved away, but when the feature was reduced using a dipole-induced strength, it gave results for H2 column densities consistent with best estimates for the sharp quadrupole lines. In studying the long path spectra of methane, that same feature was also present. A second similar problem exists with a Uranian feature--indeed, a general planetary feature centered near 6825 A.
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