Nature of quasi-stellar objects
Quasar properties from cosmological nature, discussing red shift, luminosity, radiation intensity, absorption features, distribution, chemical composition, etc
Burbidge, G. R.↗
SEARCH · Engineering Papers
Results for “RADIATION INTENSITY”
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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An interferometric approach to the measurement of optical polarization
Optical polarization, discussing radiation intensity and state measurement by two beam interferometer
Abhyankar, K. D.↗
Mean lives and relative initial state populations of some states in He II using beam-foil excitation
He II 3s and 3d states mean lives and initial population as function of energy, analyzing emitted radiation intensity
Chupp, E. L.↗
Cs2Te standard cell development and electronic characteristics of silver halides Quarterly status report, period ending 31 Oct. 1970
Production of cesium-telluride for measurement of ultraviolet radiation intensity
Spicer, W. E.↗
Search for 3.5-millimeter continuum radiation from infrared stars and related objects
IR stars and galaxies measurements, determining 3.5 mm continuum radiation intensity
Hobbs, R. W.↗
Radiative transfer effects behind reflected shock waves
Theoretical studies are reported which were largely centered on the nonequilibrium coupling of collisional, ionization, and radiative transfer processes behind reflected shock waves in nitrogen. Experimental studies included broad-band photomultiplier radiative intensity measurements, luminosity photographs of the reflected shock wave front, end-wall heat transfer measurements, and reflected shock velocity time-history measurements. The results of these activities are summarized, and comparisons between the theoretical and experimental results are discussed.
Nerem, R. M.↗
New half-range differential approximation for spherically-symmetric radiative transfer.
A new half-range differential approximation for radiative transfer with spherical symmetry is presented. The development is motivated by the various failures of existing differential approximations in determining emissive-power distributions and heat transfer for concentric-spheres problems. The new approach represents a modification of the four-moment double spherical-harmonics method, to which it reduces in the planar limit. The difference is effected by relocating the discontinuity of the assumed directional distribution of radiation intensity. The shift takes the discontinuity from precisely on the division between radially inward and radially outward, to just within the radially-outward directional half range. The method is tested on a variety of concentric spheres problems with and without internal heat sources, reproducing all the important features of the exact results.
Moreno, J. B.↗
Azimuth angle dependence of equatorial ultraviolet airglow.
An EUV solar blind photomultiplier was rocket-flown to an altitude of 103 km from Kourou, French Guiana. The rocket was spinning, thus allowing observations in all azimuthal directions within 15 deg from the horizontal plane. The observed radiation is strongly dependent on azimuth angle, the maxima of radiation are located in the southwest direction (the directions of maximum are slightly different when the experiment is looking down or up), and the radiation intensity is independent of elevation angle, suggesting that the glow is located between 75 and 105 km in altitude.
Quessette, J. A.↗
Methods of studying polarization of variable star radiation
Polarized light from variable stars can be used to determine radiation intensity and wavelength. Various types of polarization analyzers are discussed (single-beam and double-beam) as well as their modes of use (continuous and discrete). Modulation of polarizers and determination of measurement accuracy are also covered.
Shakhovskoy, N. M.↗
Broad band solar EUV absorption in the earth's upper atmosphere.
Observation data on solar radiation intensity, based on measurements performed as a function of time for three broad wavelength bands between 280 and 1030 A by a wheel spectrometer on Oso 5 during sunrise and sunset, are compared with predicted intensity variations based on Cira models. The differences between sunrise and sunset data, as well as those between observed and predicted data are discussed.
Allen, K. H.↗
Nonthermal radio observations of the major planets.
The complex and intriguing source of emission over the entire radio spectrum that Jupiter represents is reviewed in the light of ground radio observation data gathered over a period of seventeen years. The observations indicate the presence of intense radiation belts and a strong magnetic field inclined to the axis of rotation. At decametric wavelengths, several remarkably powerful sources are correlated with the rotation of the planet and the orbital motion of the satellite Io. There is at most marginal evidence of nonthermal emission from Saturn, and no such evidence as yet from Uranus and Neptune.
Smith, A. G.↗
Inference of total ozone from photometric measurements of sky radiation.
Ground-based photometric measurements of spectral sky radiation have been made using a simple filter instrument. Sky radiation intensities measured in the solar vertical at 3200 and 3600 A are compared to infer total ozone. A model of a multiple scattering Rayleigh atmosphere serves as a primary reduction parameter. Spectral measurements of all-sky radiance distribution are used to study the effects of haze and clouds on the inference of total ozone. The brightness distribution of clear and overcast sky in ultraviolet is also described.
Ghazi, A.↗
Nonthermal radio observations of the major planets
Seventeen years of observations have shown that Jupiter is a complex and intriguing source of emission over the entire radio spectrum accessible from the ground. The observations indicate the presence of intense radiation belts and a strong magnetic field inclined to the axis of rotation. At decametric wavelengths, several remarkably powerful sources are correlated with the rotation of the planet and the orbital motion of the satellite Io. Longer-term variations of these sources may be associated with the sunspot cycle, with Jupiter's orbital motion, or with changes in the internal structure of the planet. There is at most marginal evidence of nonthermal emission from Saturn, and as yet no evidence for such radiation from Uranus or Neptune.
Smith, A. G.↗
Radioisotope tracer studies in the NASA Skylab ethothermic brazing experiment M-552
The first use of radioisotope tracer for mapping flow patterns during brazing of metal components in a space environment (near-zero gravity) proved successful. A nickel ferrule was brazed to a nickel tube with Lithobraze BT (71.8% Ag, 28% Cu, 0.2% Li) which contained a trace amount of radioactive Ag-110. Mapping of the flow of the braze alloy in the annulus formed between the tube and the concentric ferrule was determined by counting the radiation intensity as a function of position in the braze joint. Significant information concerning the thermal history of the braze was determined.
Braski, D. N.↗
Environmental microbiology as related to planetary quarantine
The mechanistic basis of the synergetic effect of combined heat and radiation on microbial destruction was analyzed and results show that radiation intensity, temperature, and relative humidity are the determining factors. Dry heat resistance evaluation for selected bacterial spore crops indicates that different strains of Bacillus stearothermophilus demonstrate marked differences in resistance. Preliminary work to determine the effects of storage time, suspending medium, storage temperature and spore crop cleaning procedures on dry heat survival characteristics of Bacillus subtilis var. Niger, and dry heat resistance of natural microflora in soil particles is also reported.
Pflug, I. J.↗
Ordered structures and jet noise
A series of measurements of near field pressures and turbulent velocity fluctuations were made in a jet having a Reynolds number of about 50,000 in order to investigate more quantitatively the character and behavior of the large scale structures, and to ascertain their importance to the jet noise problem. It was found that the process of interaction between vortices can be inhibited by artificially exciting the shear layers with periodic disturbances of certain frequency. The turbulent fluctuation amplitudes measured at four diameters downstream decreased considerably. Finally, it was observed that the passage frequency of the structures decreased with x in a similar manner as the frequency corresponding to the maximum intensity radiation emanating from the same value of x.
Petersen, R. A.↗
Acceleration of isolated atoms by radiation pressure
A model is considered of a point source of radiation with a power-law spectrum in which atoms are both accelerated and photoionized by the radiation pressure, and the resulting spectrum of escape velocities is calculated. It is found that the velocity spectrum will depend only on the power-law index and will be independent of the radiation intensity. It is shown that relativistic velocities are not possible for power-law indices typical of astrophysical objects.
Gordon, R. H.↗
Main magnetic field of Jupiter and its implications for future orbiter missions
A very strong planetary magnetic field and an enormous magnetosphere with extremely intense radiation belts exist at Jupiter. Pioneer 10 and 11 fly-bys confirmed and extended the earlier ground based estimates of many of these characteristics but left unanswered or added to the list of several important and poorly understood features: the source mechanism and location of decametric emissions, and the absorption effects by the natural satellites Amalthea, Io, Europa and Ganymede. High inclination orbits (exceeding 60 deg) with low periapses (less than 2 Jupiter radii) are required to map the radiation belts and main magnetic field of Jupiter accurately so as to permit full investigation of these and associated phenomena.
Acuna, M. H.↗