Voyager 2 in the Uranian System: Imaging Science Results

@article{Smith1986Voyager2I,
  title={Voyager 2 in the Uranian System: Imaging Science Results},
  author={B. A. Smith and Laurence A. Soderblom and Reta Beebe and D. Bliss and Joseph M. Boyce and Andre Brahic and Geoffrey A. Briggs and R. Hamilton Brown and S. A. Collins and Allan F. Cook and Steven K. Croft and Jeffery N. Cuzzi and G. Edward Danielson and Merton E. Davies and Timothy E. Dowling and David Godfrey and C. Hansen and C. Harris and Garry E. Hunt and Andrew P. Ingersoll and Torrence V. Johnson and R. H. Jr. Krauss and Harold Masursky and David R. Morrison and Tobias C. Owen and Jeffrey B. Plescia and James B. Pollack and Carolyn C. Porco and Kathy A. Rages and Carl E. Sagan and Eugene Merle Shoemaker and Lawrence A. Sromovsky and C. L. Stoker and Robert Strom and Verner E. Suomi and Stephen P. Synnott and Richard Terrile and Peter C. Thomas and W. Reid Thompson and Joseph Frank Veverka},
  journal={Science},
  year={1986},
  volume={233},
  pages={43 - 64}
}
Voyager 2 images of the southern hemisphere of Uranus indicate that submicrometersize haze particles and particles of a methane condensation cloud produce faint patterns in the atmosphere. The alignment of the cloud bands is similar to that of bands on Jupiter and Saturn, but the zonal winds are nearly opposite. At mid-latitudes (-70� to -27�), where winds were measured, the atmosphere rotates faster than the magnetic field; however, the rotation rate of the atmosphere decreases toward the… 
Voyager 2 at Neptune: Imaging Science Results
Voyager 2 images of Neptune reveal a windy planet characterized by bright clouds of methane ice suspended in an exceptionally clear atmosphere above a lower deck of hydrogen sulfide or ammonia ices.
Keck Adaptive Optics Images of Uranus and Its Rings
Abstract We present adaptive optic images of Uranus obtained with the 10-m W. M. Keck II telescope in June 2000, at wavelengths between 1 and 2.4 μm. The angular resolution of the images is
Voyager 2 Radio Science Observations of the Uranian System: Atmosphere, Rings, and Satellites
TLDR
Voyager 2 radio occultation measurements of the Uranian atmosphere suggest a new kdnd of planetary ring feature characterized by highly ordered cylindrical substructures of radial scale on the order of meters and azimuthal scale of kilometers or more.
The atmosphere of Uranus: Results of radio occultation measurements with Voyager 2
During Voyager 2's occultation by Uranus the radio link from the spacecraft probed the atmosphere of the planet at latitudes ranging from 2° to 7° south. The measurements, which were conducted at two
Uranus at equinox: Cloud morphology and dynamics
Post-equinox dynamics and polar cloud structure on Uranus ☆
Uranus' Apparent Seasonal Variability in 25 HST Filters☆
Abstract Hubble Space Telescope (HST) images of Uranus taken in 1997 reveal that Voyager's view of the southern hemisphere was not representative of the rest of the planet. The banded structure with
Azimuthal brightness variation and albedo measurements of the Uranian rings
The recent Voyager encounter with Uranus has produced new insights and observational constraints on the structure, composition, and evolution of the Uranian rings. We have made careful measurements
...
...

References

SHOWING 1-10 OF 67 REFERENCES
Voyager 2 Radio Science Observations of the Uranian System: Atmosphere, Rings, and Satellites
TLDR
Voyager 2 radio occultation measurements of the Uranian atmosphere suggest a new kdnd of planetary ring feature characterized by highly ordered cylindrical substructures of radial scale on the order of meters and azimuthal scale of kilometers or more.
Infrared Observations of the Uranian System
TLDR
Estimates of phase integrals suggest that these satellites have unusual surface microstructure, which are nearly identical values at the poles and near the equator but are 1 or 2 degrees lower at mid-latitudes in both hemispheres.
Voyager 2 observations of Saturn's northern mid-latitude cloud features - Morphology, motions, and evolution
Voyager 2 images provide a basis for detailed study of the morphology and circulation of Saturn's northern mid-latitudes. Both Saturn's large-scale cloud bands and the distribution of its local cloud
Encounter with saturn: voyager 1 imaging science results.
TLDR
As Voyager 1 flew through the Saturn system it returned photographs revealing many new and surprising characteristics of this complicated community of bodies, including small inner satellites that interact gravitationally with one another and with the ring particles in ways not observed elsewhere in the solar system.
Albedo asymmetry of Iapetus
Voyager images of Saturn's moon, Iapetus1,2, confirm deductions made from Earth-based observations dating back to 1671 of a very dark leading hemisphere and a very bright trailing hemisphere3–5.
Voyager 2 Radio Observations of Uranus
TLDR
Dynamically evolving radio events of various kinds embedded in these emissions suggest a Uranian magnetosphere rich in magnetohydrodynamic phenomena.
Magnetic Fields at Uranus
The magnetic field experiment on the Voyager 2 spacecraft revealed a strong planetary magnetic field of Uranus and an associated magnetosphere and fully developed bipolar masnetic tail. The detached
A New Look at the Saturn System: The Voyager 2 Images
TLDR
Within Saturn's rings, the "birth" of a spoke has been observed, and surprising azimuthal and time variability is found in the ringlet structure of the outer B ring, leading to speculations about Saturn's internal structure and about the collisional and thermal history of the rings and satellites.
...
...