Acoustic simulation of lunar echoes.
Acoustic simulation of lunar and other rough surfaces to study electromagnetic wave reflection and scattering
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Acoustic simulation of lunar and other rough surfaces to study electromagnetic wave reflection and scattering
Lunar radar echoes depolarization studied via lunar surface backscattering characteristics at 23 cm wavelength
Ionospheric scintillations of lunar radar echo components isolation by CW Doppler shift or coherent pulse time delay techniques
Radar backscattering of lunar surface studied for circular and linear polarization of waves
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Description of lunar surface from radar lunar echoes with definition of roughness based on statistical properties of a surface
Following the idea of a fundamental station, the Wettzell Laser Ranging Station was designed to range to all types of satellites and to the moon. After obtaining the first lunar echos in October 1990, the system's operation was improved. A short report of lunar ranging activities is given.
Radar astronomical polarization measurements for lunar echoes by exploiting ionospheric Faraday rotation with linearly polarized antenna
Lunar radar echoes wavelength dependence in terms of backscattering behavior
Short-pulse radio reflections to determine average scattering behavior of lunar surface at 23 cm wavelength
Lunar radar echo measurments to determine size and electron density of earth magnetospheric wake
The intensity distribution of lunar radar echoes has been mapped for two-thirds of the earth-visible lunar surface at a wavelength of 70 cm. The depolarizing effects of the lunar surface were observed by simultaneously receiving the radar echoes in opposite polarizations. These echoes were mapped with areal resolutions of 25-100 sq km. Mapping with this resolution confirmed that the young craters have enhanced returns. A few craters were found to have enhanced echoes only from their rims. Backscattering differences were also observed between various areas within a mare, between different highland areas, and between maria and adjacent highlands. These scattering differences were interpreted with a simple model, which assumed that the surface backscattered with varying amounts of quasi-specular and diffuse power. Only an increase in the diffuse power was needed to give the numerical values of the enhancements.
Lunar radar echoes at 6 and 12 m wavelengths analyzed to obtain lunar surface scattering data
Statistical radar estimate of lunar surface roughness
Physical constants of the lunar surface as indicated by its radar scattering and thermal emission properties
Beam-width limited radar reflections from idealized Moon obtained with aid of differential reflectivity concept
Moon surface roughness estimation from analysis of 68 cm radar echoes, using geometric-optics model
Radar methods in lunar probing, discussing data obtained from surface soundings