Other
Scientific paper
May 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...213l.135m&link_type=abstract
Astrophysical Journal, Part 2 - Letters to the Editor, vol. 213, May 1, 1977, p. L135-L137. Research supported by the Battelle M
Other
1
Atmospheric Scattering, Light Emission, Optical Polarization, Planetary Atmospheres, Uranus (Planet), Haze, Light Scattering, Methane, Planetary Radiation, Polarization Characteristics, Rayleigh Scattering, Vertical Distribution
Scientific paper
The whole-disk polarization of Uranus was measured over two apparitons in blue and red light. The blue polarization becomes negative near the 0.5-deg phase, indicating non-Rayleigh scattering. The red polarization phase curve shows positive polarization smaller than suggested by Rayleigh scattering models. An explanation of these data is that the blue and red radiation is scattered by the CH4 haze layer that has been suggested to reside high in the atmosphere of Uranus. As expected, there is no whole-disk circular polarization, an observation which confirms other observations and theoretical predictions.
Michalsky Joseph J. Jr.
Stokes Robert A.
No associations
LandOfFree
Whole-disk polarization measurements of Uranus at visible wavelengths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Whole-disk polarization measurements of Uranus at visible wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Whole-disk polarization measurements of Uranus at visible wavelengths will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1882764