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- W2013005673 abstract "Images of the lunar surface were obtained at several wavelengths using a silicon vidicon imaging system and ground-based telescopes. These images were recorded and processed in digital form so that quantitative information was preserved. The photometric precision of the images is shown to be better than 1%. Ratio images calculated by dividing images obtained at two wavelengths (0.40/0.56 and 0.95/0.56 μm) are presented here for about 50% of the lunar frontside. Spatial resolution is about 2km at the sub-Earth point. A complex of distinct units is evident in the images. Earlier work with the reflectance spectrum of lunar materials indicates that for the most part these units are compositionally distinct. Digital images of this precision are extremely useful to lunar geologists in disentangling the history of the lunar surface." @default.
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- W2013005673 modified "2023-10-14" @default.
- W2013005673 title "Multispectral mapping of the lunar surface using ground-based telescopes" @default.
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- W2013005673 doi "https://doi.org/10.1016/0019-1035(76)90099-3" @default.
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