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    In:  CASI
    Publication Date: 2006-02-14
    Description: Observations were made and analyzed for Uranus, Saturn, and Titan in the continuum at the VLA and some spectroscopy at OVRO. Accurate A, B, C rings brightness temperatures from Saturn are a basis of scattering theory calculations. Variations of 2 cm limb darkening with pole orientation were modeled and are shown to originate in the deep atmosphere.
    Keywords: ASTRONOMY
    Type: NASA, Washington Reports of Planetary Astronomy, 1985; p 47-48
    Format: text
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