RADIO CHARACTERISTICS OF LUNAR SURFACE MATERIAL
Comparison of theories of radio scattering from the moon, giving the electromagnetic and the thermodynamic constants of the lunar surface
Engineering topics
Publications and source records attributed to Siegel, K. M..
Comparison of theories of radio scattering from the moon, giving the electromagnetic and the thermodynamic constants of the lunar surface
Application of millimeter wavelengths for mars mission communication offers a small advantage over conventional microwave systems
Bistatic and monostatic, multiwavelength, high resolution radar proposed for determining geometrical character and material composition of the martian surface
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Physical constants of the lunar surface as indicated by its radar scattering and thermal emission properties
Investigation of the physical properties of the lunar surface layer as simulated by terrestrial and extraterrestrial materials
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Electromagnetic parameters of meteorites, tektites, glasses, and rocks
A theory is described in which the moon is regarded as a "quasi-smooth" scatterer at radar frequencies. A scattered pulse is then composed of a number of individual returns each of which is provided by a single scattering area. In this manner it is possible to account for all the major features of the pulse, and the evidence in favor of the theory is presented. From a study of the measured power received at different frequencies, it is shown that the scattering area nearest to the earth is the source of a specular return, and it is then possible to obtain information about the material of which the area is composed. The electromagnetic constants are derived and their significance discussed.