Ganymede: Radar Surface Characteristics
暂无分享,去创建一个
Radar observations of Ganymede, at X-band, show that the surface is unusually bright and has unusual polarization properties. A model of the surface based on large numbers of random ice facets (hence vacuum-ice interfaces) is able to account for these characteristics.
[1] Donald B. Campbell,et al. Galilean satellites: 1976 radar results , 1978 .
[2] U. Fink,et al. Infrared spectra of the Galilean satellites of Jupiter , 1973 .
[3] Gordon H. Pettengill,et al. Icy craters on the Galilean satellites , 1978 .
[4] P. H. Smith. Diameters of the Galilean satellites from pioneer data , 1978 .
[5] G. W. Null,et al. Gravity field of Jupiter and its satellite from Pioneer 10 and Pioneer 11 tracking data , 1976 .