Interstellar absorption and color excesses in Sco OB-1
Interstellar absorption and color excesses in Sco OB-1 from spectral observation and photometry for star cluster and association background
Engineering topics
Publications and source records attributed to Westphal, J. A..
Interstellar absorption and color excesses in Sco OB-1 from spectral observation and photometry for star cluster and association background
Mars IR spectral geometric albedo of bright and dark regions for surface composition model
System will collimate and direct an argon laser beam with high angular tracking accuracy at objects on the moons surface. It can be adapted to missile and satellite tracking.
Local thermal emission from Jupiter at 5 microns, discussing North Equatorial Belt and atmospheric transparency
IR and optical measurement of Crab pulsar NP 0532, analyzing energy density per pulse and smoothness of visual data
IR observations of ETA Carinae to 20 microns, noting continued increase in flux density into IR
Photoelectric monitoring broadband photometry and spectral scans of candidate star for pulsating radio source CP 1919
Photometric data extending continuum observations for nonstellar object eta Carinae, discussing energy distribution and IR properties
IR observations of comet 1965f show color temperature changes with solar distance
Spectral emissivity difference measurement method for region between two points on lunar surface, discussing applications to bright planets
IR thermal emission from lunar nighttime surface, noting anomalies location and observational procedure
IR photometric measurement of Comet 1965f, noting absolute intensity dependence on distance from Sun, tail intensities and nature of particle emissions
Limb darkening measurements of Venus at 8-14 microns with 200 inch Hale telescope
Thermal 8-14 micron IR emission of Jupiter in December 1963
Cooling and reheating of Jupiter satellite Ganymede when disappearing and reappearing from Jupiter shadow observed at Palomar Observatory
Brightness temperature distribution across jupiter disk and integral brightness temperatures of galilean satellites mapped from observations at 10 microns with 200-inch hale telescope
Venus - high resolution map of brightness temperature from hale telescope observations