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- W2287458020 abstract "We model radar scattering by planetary surfaces using a ray-optics algorithm that includes Fresnelian reflection and refraction, diffuse scattering, and coherent backscattering. We enhance the realism of the ray-optics algorithm by using scattering particles that are geometrically representative of the surfaces and interiors of planetary bodies. The shapes as well as the dielectric properties of the scattering particles have been characterized in laboratory. The results demonstrate the effects of various physical parameters on radar scattering with an emphasis on asteroids. We present the effects of number density, size distribution, and dielectric and geometric properties of scattering particles on the radar reflectivity and circular-polarization ratio of planetary surfaces. We also briefly discuss applications to the Galilean Moon Europa and comets." @default.
- W2287458020 created "2016-06-24" @default.
- W2287458020 creator A5002639269 @default.
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- W2287458020 date "2016-05-01" @default.
- W2287458020 modified "2023-10-18" @default.
- W2287458020 title "Radar scattering by planetary surfaces modeled with laboratory-characterized particles" @default.
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- W2287458020 doi "https://doi.org/10.1016/j.icarus.2016.01.011" @default.
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