The southern sky survey payload
Measurements on ultraviolet fluxes from stars and nebulosities by rockets carrying photomultiplier and ionization chamber detectors
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Measurements on ultraviolet fluxes from stars and nebulosities by rockets carrying photomultiplier and ionization chamber detectors
UV color and flux at 2200 and 2600 angstroms measured for A and B stars, using rocketborne photometers
Millimeter wavelength brightness temperatures of Mars, Jupiter and Saturn calculated from antenna temperatures
Photoelectric observations and orbital solutions of BV 267, obtaining new light elements, system light change and orbital solutions
Rapid drift in longitude of small dark spot on south edge of Jupiter North Temperate Belt, noting sinusoidal displacement characteristics and measurement with blue and UV photography
Lunar photometric brightness variational function based on JPL study of Moon topology
Optical photometric properties of lunar surface, discussing brightness effects, solar wind, albedo, reflectivity, backscatter, chemical composition, ion bombardment effects, etc
Multicolor photometric work on bright stars by Lunar and Planetary Laboratory
IR photometric measurement of Comet 1965f, noting absolute intensity dependence on distance from Sun, tail intensities and nature of particle emissions
Martian surface markings, brightness along optical equator, crater erosion, asteroid collision and yellow dust clouds
Intensity microphotometer design in which input signal is converted by piecewise-linear diode approximators
Optical identification of position of X-ray astronomical source Sco X-1, noting similarity of certain properties with old novae
Directional absorptivity characteristics of conical cavities and use as thermal model for lunar meteor craters
Classification of slit spectrograms of 185 bright stars in Morgan-Keenan system
Photoelectric two-cell polarimeter with rotating achromatic half-wave plane noting wavelength restriction
OH emission in H II region W3, using improved equipment
Multichannel photometer for space applications requiring low weight and power, no moving parts and high sensitivity divided in four electrically and optically distinct quadrants