Extra-atmospheric Measurements of the Ultraviolet and X-ray Backgrounds and Their Role in the Study of Intergalactic Gas
Ultraviolet and X ray background extraatmospheric measurements and role in study of intergalactic gas
Kurt, V. G.↗
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X-radiation of the moon and Roentgen cosmic background according to data of AMS ''Luna-12''
Satellite measurements of lunar soft X radiation, and Roentgen cosmic background
Cheremukhin, G. S.↗
Two-twenty Kev Spectrum of X-rays from the Crab Nebula and the Diffuse Background near Galactic Anticenter
X ray spectroscopy of Crab nebula and diffuse background by sounding balloons and rockets
Boldt, E. A.↗
Cosmology, black-body radiation, and the diffuse X-ray background.
Relativistic electron energy loss due to inverse Compton scattering from cosmological blackbody radiation, noting diffuse X ray background implication for electron source strength
Brecher, K.↗
Detection of an anisotropic soft X-ray background flux.
Anisotropic soft X ray background flux detection, discussing extragalactic and possible galactic corona components
Bowyer, C. S.↗
The diffuse X-ray background.
Isotropic X ray background in space, discussing galactic contributions and evolutionary effects
Silk, J.↗
Reduction of cosmic background in an X-ray proportional counter through risetime discrimination.
Cosmic ray background radiation reduction by risetime discrimination applied to proportional counter for sounding rocket X ray astronomy
Gorenstein, P.↗
Wave propagation in a random medium with stratified background.
Wave propagation in stratified medium with random background using Fourier-Stieltjes spectral representation
Liu, C. H.↗
Monopole mass spectrometer with improved sensitivity and reduced background
Monopole mass spectrometer is increased by nearly an order of magnitude when a weak external magnetic field is applied so that the ion beam is deflected towards the rod. This magnetic field eliminates background noise at the low end of the mass scale.
Herzog, R. F.↗
Evaluation of the acoustic sources of background noise in wind tunnel facilities
Methods for determining acoustic sources of background noise in wind tunnels
Source record↗
Background of piloted simulator development
Background of piloted simulator development
Westbrook, C. B.↗
Night sky background conditions and launch windows for research experiments
Computer program for launch window determination from star illumination of night sky background
Keating, J. C.↗
Two-twenty keV X-ray sky background
X ray spectra of diffuse sky background in 2-20 keV range
Boldt, E. A.↗
Diffusion of electron plasma oscillations in a large-amplitude ion-wave background.
Electron plasma oscillations diffusion due to scattering by large amplitude ion wave background, noting electron wave spectrum evolution
Davidson, R. C.↗
Detection time to a point source of light appearing on a star field background with and without a glare source present.
Detection time to light point source noting response to dark, star field and glare source backgrounds
Haines, R. F.↗
Upper limits to the intensity of background radiation at lambda equals 1.32, 0.559, and 0.359 mm.
Background radiation intensity upper limits for mm and submillimeter wavelengths in interstellar medium, noting intense flux in far IR
Bortolot, V. J., Jr.↗
The effect of background pressure and magnetic field shape on MPD thruster performance.
Background pressure and magnetic field shape effect on MPD thrustor performance, testing radiation cooled thrustors
Connolly, D. J.↗
High-energy gamma rays, cosmic-ray electrons, and the far-infrared background radiation.
Inverse compton scattering of far IR background radiation proposed as explanation of high energy gamma ray flux
Shen, C. S.↗