CCD spectroscopic observations of Saturn, Uranus, Neptune, and Titan during the 1990 apparitions
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference32 articles.
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3. The atmospheric structure and dynamical properties of Neptune derived from ground-based and IUE spectrophotometry;Baines;Icarus,1990
4. Absolute spectrophotometry of Neptune: 3390 to 7800 Å;Bergstralh;Icarus,1983
5. A study of the atmosphere of Saturn based on methane line profiles near 1.1 μm;Buriez;Astron. Astrophys.,1981
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1. Atmospheric studies with spectro-imaging : prospects for the vims experiment on Cassini;Planetary and Space Science;1998-10
2. Saturn 1991–1993: Clouds and Hazes;Icarus;1996-01
3. Spectrophotometry of the Jovian Planets and Titan at 300- to 1000-nm Wavelength: The Methane Spectrum;Icarus;1994-09
4. Saturn's Upper Atmospheric Hazes Observed by the Hubble Space Telescope;Icarus;1993-12
5. Absolutely calibrated CCD images of Saturn at methane band and continuum wavelengths during its 1991 opposition;Journal of Geophysical Research: Planets;1993-02-25
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