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  • 1
    Publication Date: 2005-11-30
    Description: Infrared and radar studies of the Apollo 16 landing site are summarized. Correlations and comparisons between earth based remote sensing data, IR observations, and other data are discussed in detail. Remote sensing studies were devoted to solving two problems: (1) determining the physical difference between Cayley and Descartes geologic units near the landing site; and (2) determining the nature of the bright unit of Descartes mountain material.
    Keywords: SPACE SCIENCES
    Type: NASA. Lyndon B. Johnson Space Center Apollo 16 Prelim. Sci. Rept.; 5 p
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  • 2
    Publication Date: 2006-01-11
    Description: An examination was made of earth based observations of optical color differences, infrared eclipse temperatures, and radar backscatter for Mare Serenitatis. Information is also included on orbital observations, physical properties of surface types, and correlation of surface types with geologic units. Differences in these remote observations are attributed to variations in chemical and minerological compositions.
    Keywords: SPACE SCIENCES
    Type: NASA. Johnson Space Center Apollo 17 Prelim. Sci. Rept.; 7 p
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  • 3
    Publication Date: 2011-08-16
    Description: Radar reflectivity correlations with lunar surface structure in Mare Imbrium, using delay-Doppler radar maps
    Keywords: SPACE SCIENCES
    Type: ; 37 (
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  • 4
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: Lunar radar reflectivity mapping at 7.5 m wavelength for maria and highlands echo powers, using interferometric techniques
    Keywords: SPACE SCIENCES
    Type: ; TROPHYSICAL JOURNAL
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  • 5
    Publication Date: 2011-08-16
    Keywords: SPACE SCIENCES
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  • 6
    Publication Date: 2011-08-12
    Description: Radar echoes intensity distribution maps from lunar surface surrounding crater Tycho
    Keywords: SPACE SCIENCES
    Type: ; TA FREQUENZA (
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  • 7
    Publication Date: 2013-08-31
    Description: Three sets of polarized radar-echo images of the Moon were examined to establish the relation between radar resolution and landform-identification resolution. After comparison with lunar maps and photographs, real and apparent landforms on the radar images were grouped into one of seven classes. Results show strong relations between radar resolution and diameter or relief of landforms that are clearly identified and those that would probably be correctly identified (class 1 and class 2). Landforms are not detected (class 5) at all diameters and reliefs, but the percentage of undetected landforms decreases with increasing mean diameter and mean relief. Landforms are simply detected (class 4) at most mean diameters and reliefs. Ambiguous arrays (class 6) portrayed by the radar constitute up to about 16, 22, and 15% of the landforms at various diameters and relief values for the 3.8 cm, 70 cm high resolution, and 70 cm low resolution images, respectively. Only a few percent of the landforms portrayed by the radar images at various diameters and relief values are fictitious (class 7).
    Keywords: EARTH RESOURCES AND REMOTE SENSING
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 240-242
    Format: application/pdf
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  • 8
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    In:  CASI
    Publication Date: 2013-08-31
    Description: Previous radar mappings of the Moon at 70 cm wavelength in the late 1960's by Thompson have been replaced with a new set of observations using the 430 MHz radar at the Arecibo Observatory, Puerto Rico. Radar resolution was reduced to 2 to 5 km radar cell size and a beam-sweep, limb-to-limb calibration was conducted. Advances in computer technology provided the principle means of improving lunar radar mapping at this wavelength. Observation techniques and data processing are described and scattering differences found in the orthographic projection of the radar data are discussed.
    Keywords: EARTH RESOURCES AND REMOTE SENSING
    Type: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986; p 238-239
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  • 9
    Publication Date: 2019-06-28
    Description: The NASA/JPL aircraft synthetic aperture radar (SAR) was used to conduct major data acquisition expeditions in 1983 through 1985. Substantial improvements to the aircraft SAR were incorporated in 1981 through 1984 resulting in an imaging radar that could simultaneously record all four combinations of linear horizontal and vertical polarization (HH, HV, VH, VV) using computer control of the radar logic, gain setting, and other functions. Data were recorded on high-density digital tapes and processed on a general-purpose computer to produce 10-km square images with 10-m resolution. These digital images yield both the amplitude and phase of the four polarizations. All of the digital images produced so far are archived at the JPL Radar Data Center and are accessible via the Reference Notebook System of that facility. Sites observed in 1984 and 1985 included geological targets in the western United States, as well as agricultural and forestry sites in the Midwest and along the eastern coast. This aircraft radar was destroyed in the CV-990 fire at March Air Force Base on 17 July 1985. It is being rebuilt for flights in l987 and will likely be operated in a mode similar to that described here. The data from 1984 and 1985 as well as those from future expeditions in 1987 and beyond will provide users with a valuable data base for the multifrequency, multipolarization Spaceborne Imaging Radar (SIR-C) scheduled for orbital operations in the early 1990's.
    Keywords: EARTH RESOURCES AND REMOTE SENSING
    Type: NASA-CR-180237 , JPL-PUB-86-20 , NAS 1.26:180237
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  • 10
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: Comparison of anomalous behavior at infrared and radar wavelengths provides an estimation of lunar surface structure at centimeter-to-meter sizes. Although a simple classification is used, it is shown that the combination of the infrared and radar data contains more information than any of the sets by themselves. The infrared data indicate that bare surface rocks are the source of the roughness which generates enhanced radar backscatter. The different radar maps indicate the size of surface rocks, as was demonstrated for the strewn fields of centimeter-sized rubble (the Type II anomaly). As craters age, they have a rim-bright appearance in the radar maps, and eventually lose their anomalous-behavior at infrared and 3.8-cm radar wavelengths.
    Keywords: SPACE SCIENCES
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