A readily available material for the simulation of lunar optical properties.
Lunar optical properties simulated with commercial Portland cement and maroon and black coloring powders, noting blue-green color index discrepancy
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Lunar optical properties simulated with commercial Portland cement and maroon and black coloring powders, noting blue-green color index discrepancy
Optical properties of Martian surface indicate redness results from high atmospheric absorption
Optical properties of zinc oxide analyzed by exposing samples to mechanical and thermal treatments and UV radiation
Quenched MnBi thin films measured for magnetic, magneto-optical and optical properties, noting Faraday rotation
Alteration of surface optical properties by high speed micron-size particles
Optical properties of zinc oxide analyzed by exposing samples to mechanical and thermal treatments and UV radiation
Optical properties of Mo, Ta W and Re by reflectance vs incidence angle method, stressing dielectric constants
Optical properties of lunar powder samples from Tranquility Base
Fluorel L-3203-6 and 1059 and four Fluorel derivatives were irradiated monochromatically and hemispherically with electromagnetic energy in the solar- and infrared-wavelength range to determine the thermal-optical properties that are required for engineering analysis. The thermal-optical properties were measured and analyzed, and the resulting data were tabulated for convenient engineering use. The results prove that the electromagnetic-energy distribution and the measured reflectance and transmittance of materials can be used to calculate several mean values, which are the total and hemispherical thermal-optical properties. The test results also illustrate that Fluorel effectively absorbs energy in the solar- and infrared-wavelength range. In addition, the results demonstrate that fabrication alters the thermal-optical properties of Fluorel.
Chemical, electrical, and optical properties of cobalt as gallium phosphide impurity
Metallurgical, electrical, and optical properties of gallium phosphide
Relationships between the inherent and optical properties of the ocean (Gorden et al., 1975 and Preisendorfer, 1961) are combined with the Duntley-Preisendorfer equation to show the dependence of these properties on the depth at which a Secchi disk disappears from view. An expression relating the Secchi depth to the limiting contrast of the disk is derived in terms of the average beam attenuation coefficient, the average diffuse attenuation coefficient for downwelling irradiance, the albedo of the disk, and the reflectance functions at the Secchi depth and just below the surface. It is shown that combining Secchi depth observations with other optical properties yields significant information about the constituents of the medium.
Studies of metallurgical, electrical, and optical properties of gallium phosphide
Far infrared optical properties of spacecraft paints
Lunar surface composition inferred from optical properties, comparing lunar crust with rock and meteorite powders characteristics
Lunar surface optical properties and IR emission