Optimum wavelength intervals for surface temperature radiometry.
Optimum wavelength intervals for surface temperature radiometry from total reflectance measurement of common surface minerals
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Optimum wavelength intervals for surface temperature radiometry from total reflectance measurement of common surface minerals
Millimeter wavelength solar radiation consisting of thermal, slowly varying active and burst components and eclipse measurements of brightness distribution
Solar extinction measurements and interpretation of terrestrial atmosphere microwave absorption spectrum near 1-cm wavelength
Plane interstellar polarization dependence on wavelength observed in 18 stars with UV and IR FILTER
Wavelength dependence of polarization by small graphite flakes with anisotropic dielectric constant
A thin-window proportional counter tube of 0.25-mil Mylar with a thin aluminum coating on one side permits efficient detection of long wavelength X rays. It is sufficiently rugged for long-term use in space or other demanding environments.
Radiometer instrumentation of 16-foot millimeter wavelength antenna system
Short-pulse radio reflections to determine average scattering behavior of lunar surface at 23 cm wavelength
24 hr history of radar angel activity at 3.2, 10.7 and 71.5 cm wavelengths
Radiometric maps of brightness temperature contours on lunar disk from measurements of 3.3 mm wavelength thermal emission
Absorption wavelengths of QSOs, noting relatively large red shifts
Performance characteristics of single wavelength liquid-metal MHD induction generator with end- loss compensation
Radiometric observations of total lunar eclipse of December 19, 1964 at wavelength of 3.3 mm indicate no significant temperature difference
Aperture efficiency of Parkes radio telescope reflector for decimeter and centimeter wavelengths obtained through celestial radio source
Carbon dioxide laser as a simple portable unit generates coherent light pulses at selected infrared wavelengths. The improved laser was designed for the detection of air pollutants but can be applied to optical communications.
Radio Astronomy Explorer satellite radiometer for measuring cosmic noise in vicinity of 100 meter wavelengths
Lunar radar echoes at 6 and 12 m wavelengths analyzed to obtain lunar surface scattering data
Spectral lines of spontaneous emission from helium-neon laser as convenient wavelength standard