Computer Science
Scientific paper
Feb 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988icar...73..227k&link_type=abstract
Icarus (ISSN 0019-1035), vol. 73, Feb. 1988, p. 227-247.
Computer Science
20
Albedo, Atmospheric Circulation, Equatorial Regions, Saturn Atmosphere, Spatial Distribution, Ammonia, Methane, Spectrophotometry, Spectrum Analysis, Voyager 1 Spacecraft, Saturn, Longitude, Atmosphere, Equatorial Regions, Spacecraft Observations, Voyager 1 Mission, Earth-Based Observations, Analysis, Models, Scattering, Reflectivity, Stratosphere, Haze, Spectra, Optical Properties, Albedo, Abundance, Gases, Methane, Mixing, Composition, Ammonia, Parameters, Data, Diagrams, Calculations, Radiative Transfer,
Scientific paper
Longitudinal variations in the equatorial regions of Saturn are sought in both Voyager orange and methane-filter and ground-based 6000-6600 A observations. The spectral variations found are inconsistent with reflecting layer height variation; they are alternatively modeled by changes in the single-scattering albedo of the haze, as well as in the specific abundance of haze gas. The 500-km spatial resolution data furnished by Voyager are found to be consistent with a specific abundance of haze gas between 10 and 24 km-am. Ammonia and methane mixing ratios are derived.
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