Small-angle scattering of celestial x-rays by interstellar grains.
Small angle scattering of X-rays by interstellar grains in light of neutron star discoveries
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Small angle scattering of X-rays by interstellar grains in light of neutron star discoveries
Effect of alloying on grain refinement of electron-beam-melted tungsten
Exploratory investigation of nylon grain size effect on ablation of phenolic nylon
Synthesis and analysis of ethylene-neohexene copolymers with other non ketene-imine group free radicals for solid and hybrid grain propellant saturated hydrocarbon binder program
Saturated hydrocarbon polymeric binder for advanced solid propellant and hybrid solid grains
Metal grains in 34 chondritic meteorites examined by electron microprobe
Grain size effects on tensile and creep properties of arc-melted and electron-beam-melted tungsten
Saturated hydrocarbon polymeric binder materials prepared for advanced solid propellant and hybrid solid grain
Graphite grain formation in cool stars examined on basis of molecular equilibrium data for stellar atmospheres
Far UV extinction curve and wavelength dependence of interstellar polarization by graphite grains
Metal addition effect on grain growth of matrix oxides, noting inhibitive results in most cases
Optical properties of interstellar grains, noting complex index of refraction as function of wavelength
Influence of grain-size purity relation beryllium fabrication and resulting mechanical properties
Atomic structure and chemical composition influence on grain boundaries effect on mechanical failure in polycrystalline ceramics
Grain configuration for solid propellant rocket engines
Effect of three surface finishes of roughness 4 to 5, 20 to 25, and 70 to 80 micro inches rms on fatigue properties were determined for low-carbon N-155 alloy of grain size A.S.T.M. 1 at temperatures of 80 , 1000, 1350, and 1500 F. The fatigue properties for the various finishes differed appreciably at room temperature; however, after short periods at 1000 F and for all periods investigated at temperatures above 1000 F, the specimen finishes had the same fatigue strength. It was concluded that the primary cause of the difference in room-temperature strength was due to compressive stresses set up in the surface and that at elevated temperatures these compressive stresses were relieved by annealing. Apparently, roughness alone did not significantly affect fatigue strength.
High purity, cylindrical castings of high melting point materials such as tungsten and tungsten alloys
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