Radar echoes from the icy Galilean satellites are unique in character and they may be explained by a phenomenon that was called the radar glory effect. The radar glory backscattering from buried craters was analyzed as a possible model for this effect. These craters have a smaller refractive index below the crater than above. The possibility exists that the rays will be totally internally reflected at the crater walls. The rays which contribute to the backscattering will come from a circular annulus, when viewed before the refraction occurs at the ice-vacuum surface, in a plane orthogonal to the rays reflected from the crater
The Apollo 15, 16, and 17 core tubes show that the uppermost few meters of the lunar regolith are in...
ii iv We map the planet Mercury and Jupiter’s moons Ganymede and Callisto using Earth-based radar te...
The lunar surface material in the Plato area is characterized using Earth based visual, infrared, an...
The icy moons of Jupiter were the first to show unusual radar backscatter behavior in Earth-based ex...
For lunar orbital synthetic aperture radars, such as the Chandrayaan Mini-RF operating at S- band (1...
Studies of the moon during the period of the grant revolved around the issues of the possible presen...
International audienceThe recent Cassini RADAR Enceladus E16 data reveal a tectonically-complex surf...
International audienceThe recent Cassini RADAR Enceladus E16 data reveal a tectonically-complex surf...
The initial radar observations of the mainbelt asteroids 9 Metis, 27 Euterpe, and 60 Echo are examin...
Airborne radar images of part of the Greenland ice sheet reveal icy terrain whose radar properties a...
A number of planetary objects exhibit large radar reflectivity and polarization ratios, and more rec...
In Miniature Radio Frequency (Mini‐RF) radar images, anomalous craters are those having a high circu...
The aim is to make radar reconnaissance of near-Earth asteroids, mainbelt ateroids, the Galilean sat...
During the Clementine 1 mission, a bistatic radar experiment measured the magnitude and polarization...
We reexamined our radar scattering model for young, rough craters [1] based on unpublished data from...
The Apollo 15, 16, and 17 core tubes show that the uppermost few meters of the lunar regolith are in...
ii iv We map the planet Mercury and Jupiter’s moons Ganymede and Callisto using Earth-based radar te...
The lunar surface material in the Plato area is characterized using Earth based visual, infrared, an...
The icy moons of Jupiter were the first to show unusual radar backscatter behavior in Earth-based ex...
For lunar orbital synthetic aperture radars, such as the Chandrayaan Mini-RF operating at S- band (1...
Studies of the moon during the period of the grant revolved around the issues of the possible presen...
International audienceThe recent Cassini RADAR Enceladus E16 data reveal a tectonically-complex surf...
International audienceThe recent Cassini RADAR Enceladus E16 data reveal a tectonically-complex surf...
The initial radar observations of the mainbelt asteroids 9 Metis, 27 Euterpe, and 60 Echo are examin...
Airborne radar images of part of the Greenland ice sheet reveal icy terrain whose radar properties a...
A number of planetary objects exhibit large radar reflectivity and polarization ratios, and more rec...
In Miniature Radio Frequency (Mini‐RF) radar images, anomalous craters are those having a high circu...
The aim is to make radar reconnaissance of near-Earth asteroids, mainbelt ateroids, the Galilean sat...
During the Clementine 1 mission, a bistatic radar experiment measured the magnitude and polarization...
We reexamined our radar scattering model for young, rough craters [1] based on unpublished data from...
The Apollo 15, 16, and 17 core tubes show that the uppermost few meters of the lunar regolith are in...
ii iv We map the planet Mercury and Jupiter’s moons Ganymede and Callisto using Earth-based radar te...
The lunar surface material in the Plato area is characterized using Earth based visual, infrared, an...