Photometric investigations of simulated lunar surfaces.
Photometric investigations of simulated lunar surfaces confirm high porosity and low albedo without postulating necessity for fine dust layer
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Photometric investigations of simulated lunar surfaces confirm high porosity and low albedo without postulating necessity for fine dust layer
Slope derivation from lunar orbiter photography using photometric model and computer program
PAGEOS 1 and Echo 1 satellites tracked and photometrically analyzed in U-B-V spectral regions, describing phototubes, filters and Cassegrain reflecting telescope
Photometric properties of lunar surface target areas from high resolution TV pictures received from Surveyor 1 spacecraft
Prelaunch photometric calibration of Surveyor TV system for reconstruction of lunar terrain televised pictures permitting system lunar performance prediction
Design specifications for low cost photometric telescopes
Diffraction theory of shadow knife and slit photometric methods
Stellar photometric data for six photocathode materials and silicon detector
Far ultraviolet photometric observation of intense extraterrestrial sources at 296 kilometers
Power spectrum analysis of photometric observations of white dwarf stars for measuring variability of stellar luminosity
Diffraction theory of shadow knife and slit photometric methods
Photometric and polarimetric properties of Apollo 12 and Surveyor 3 landing sites
Icarus asteroid rotation period and brightness variation values obtained from photometric observations at Cassegrain reflector focus
Photometric reduction of Lunar Orbiter video magnetic tapes for generation of topographic information of proposed Apollo landing sites
Prelaunch photometric calibration of Surveyor TV system for reconstruction of lunar terrain televised pictures permitting system lunar performance prediction
Photometric error analysis and optimum use of photomultipliers, discussing pulse-height spectra, detection and weighting systems
Venus halo and photometric evidence for ice in Venus clouds
Computer subroutines to determine photometric magnitudes of planets and their satellites