Visible spectral reflectance measurements (0.33–1.1 μm) of the Galilean satellites at many orbital phase angles
- 30 November 1980
- Vol. 44 (2) , 410-430
- https://doi.org/10.1016/0019-1035(80)90034-2
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Io: Longitudinal Distribution of Sulfur Dioxide FrostScience, 1980
- The Galilean satellites: New near-infrared spectral reflectance measurements (0.65–2.5 μm) and a 0.325–5 μm summaryIcarus, 1980
- Infrared spectrum of Io, 2.8–5.2 μmIcarus, 1980
- Spectral evidence for sublimates and adsorbates on IoNature, 1979
- Significance of absorption features in Io's IR reflectance spectrumNature, 1979
- Spectral reflectivities of the Galilean satellites and Titan, 0.32 to 0.86 micrometersIcarus, 1978
- Near-infrared spectra of the Galilean satellites: Observations and compositional implicationsIcarus, 1978
- Four-color photometry of the Galilean satellitesIcarus, 1974
- Galilean satellites the spectral reflectivity 0.30–1.10 micronIcarus, 1970
- A Double Beam Astronomical PhotometerApplied Optics, 1968