Computer Science
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...83..494n&link_type=abstract
Icarus (ISSN 0019-1035), vol. 83, Feb. 1990, p. 494-499.
Computer Science
17
Arsenic Compounds, Atmospheric Composition, Hydrides, Jupiter Atmosphere, Abundance, Atmospheric Models, Planetary Atmospheres, Jupiter, Abundance, Arsenic, Earth-Based Observations, Atmosphere, Aircraft Observations, Spectra, Comparisons, Kao Aircraft, Procedure, Models
Scientific paper
Both ground-based and airborne observations of the AsH3 Q-branch at 2126/cm, in conjunction with newly-analyzed laboratory comparison spectra at AsH3, are employed in the derivation of a new estimate of Jovian As abundance. The mole fraction on AsH3 in the Jovian atmosphere is 0.22 + or - 0.11 ppb; this is merely 0.5 times the solar abundance, and a factor-of-9 less than the mole fraction found in Saturn, duplicating the pattern noted in the relative abundance of P in these two planets and furnishing a useful constraint for models of heavy element incorporation in the outer planets' gaseous envelopes.
Geballe Thomas Ronald
Larson Harold P.
Noll Keith S.
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