Abstract Analysis of polarimetric observations of Saturn was carried out. In the long wave-length spectral range (λ > 0.5μm) polarimetric observations do not contradict the model of spherical or irregular randomly oriented particles. In the short wave-length spectral interval (λ < 0.5μm) it is necessary to take into account the scattering by oriented particles.
Physical characteristics of the upper layers of Saturn's atmosphere
Advances in Space Research ; 1 , 8 ; 183-186
01.01.1981
4 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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