Major victory for Soviet science. New data on the invisible side of the moon
Television equipment on Zond III for transmitting photographs of far side of moon - U.S.S.R.
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Television equipment on Zond III for transmitting photographs of far side of moon - U.S.S.R.
Selenographic and geologic interpretations of lunar photographs from Ranger Block III
Production and publication of Ranger Block III LUNAR photographs from film and magnetic tape
Parameters for interpretation of selected Ranger IX photographs
History, background and purpose of Ranger missions to Moon, including spacecraft, television subsystem, testing and calibration
Photometric method for deriving lunar surface elevation information from single picture
NASA Lunar Orbiter program to place unmanned spacecraft into orbit around Moon
Luna IX photographs indicate lunar surface composition of weakly cohesive poorly sorted fragmental material of unknown source
Readout and evaluation of lunar photographs taken by orbiting lunar spacecraft
Improved rapid processing methods for handling large amounts of photoclinometric data, and maximizing ratio of work done by computer relative to manual reduction
Lunar AIMP photographic data processing system which transforms photographic scans of moon into rectified lunar pictures, particulary ground processor system
Lunar optical properties simulated with commercial Portland cement and maroon and black coloring powders, noting blue-green color index discrepancy
Lunar topological photography from Surveyor 7 mission
High resolution strip photography of lunar surface
Lunar Apennine-Hadley region geological implications from high resolution earth-based radar map and Lunar Orbiter photography
Hadley Rille is directly related to the emplacement of mare basalts in Palus Putredinis. Existing hypotheses of sinuous rille origin are in discord with the cooling behavior of deep lava flows and the strength of materials. It is proposed that Hadley Rille is a channel which returned lava to the southern vent from which it initially extruded and that the channel persisted through many episodes of volcanism. This view is supported by available topographic information obtained by the lunar orbiter photography and the Apollo 15 mission.