BASIC RESEARCH ON ROCKET PROPELLANTS. MINOR COMPONENT CALCULATIONS OF CARBON, HYDROGEN, OXYGEN, AND NITROGEN
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Radiation induced changes in semiconductor materials from 40 MeV proton radiation determined by improved infrared method
D region electron density profiles and corpuscular radiation measured by DC probe and Geiger counter
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Pulse modulator is capable of continuously variable pulse width over a 10 to 1 range of 1.0 microsecond to 0.1 microsecond and operates over a wide range of pulse repetition rates. Pulse width diversity is obtained by operating step-recovery diodes in the reverse conduction mode.
Long-period librations of Trojan planetary orbits in rotating three-body coordinate system
Manganese, silicon, and magnesium markedly reduce the tendency of Inconel 718 to weld microfissuring. By combining a manganese, 0.20 percent by content, with silicon, greater than 0.25 percent content, or by adding 20 ppm of magnesium, the weld microfissuring decreased in the standard alloy.
Light curve set for Vesta obtained and compared with previous observations, discussing probable spherical shape deduction
Number densities of hydrogen species in hydrogen plasma - tables
Atmospheric component effects on attenuation of infrared radiation
Light curves for Vesta compared and rotation derived from aspect change effect on rotational period
Mn, S and rare earth additions influence on Inconel alloy weld microfissuring including material, hot ductility and tensile strength data
Lightcurves for 624 Hektor with Radcliffe, Kitt Peak, Catalina and Cerro Tololo reflectors, noting asteroid shape and rotational axis
Icarus asteroid positions, UBV magnitude, brightness, colors, light curves and polarization, noting stony-iron composition
Lydia asteroid observations, presenting light curves brightness and phase functions near opposition
Venusian photochemistry, discussing hydrogen source from HCl, loss of water in relation to HCl, carbon dioxide stability and COS and hydrogen sulfide in visible clouds
Astronomical observations of the asteroids are discussed. The origin of asteroids and their interrelationships with comets, meteorites, and meteors are considered. Possible space missions and further topics of research are also discussed.