NASA NTRS · 20040139300
[Chemistry in Outer Solar System and Beyond]
Abstract
During the three years of the NASA Planetary Atmospheres grant NAG51 1032, we have developed photochemical models for Jupiter, Saturn, Uranus, Neptune, Io, and extrasolar giant planets. We have compared the Io and outer planet model predictions with various infrared and microwave observations.
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2004-01-01. [Chemistry in Outer Solar System and Beyond]. https://ntrs.nasa.gov/citations/20040139300
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