Investigation of the detectivity of radiation- produced defect levels in n and p type silicon and germanium Semiannual progress report
Black body responsivity data of n-type and p-type silicon
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Black body responsivity data of n-type and p-type silicon
Cryogenic black body used in spectral emittance of rocks
Thermodynamic aspects of ray invariance of spectral brightness ratio to square of local index of refraction compared to black body power radiation
Unusual IR object IRC plus 10216 interpreted as galactic source surrounded by optically thick dust shells, noting resemblance to black body energy distribution
Tungsten strip lamps spectral radiance calibration, discussing accuracy requirements for radiation constants, wavelength and black body temperature
Black body cavity type radiometers for high accuracy measurement of irradiance
Reflectance measurements of directional spectral emittance of black body cavities with specific geometries, using laser source and integrating hemi-ellipsoid
Stepwise linear regressions method for estimating black body surface radiances from model atmospheres and corresponding simulated Nimbus 2 window-channel radiances
Spectral absorption of 2.7 micron water vapor band under various high temperature and pressure conditions, using black body radiation
Black body cavity radiometer with thermal resistance wire bridge circuit
Black body radiometer design with temperature sensing and cavity heat source cone winding
Zoning techniques applied to gray gas and black body radiation transport models including view effects and nonisothermal emission
IR stellar object HD 45677, discussing IR spectral energy distribution in terms of black body temperature range
Circinus pulsating X ray source spectrum analysis, considering bremsstrahlung and black body models
Highly compact X ray source spectrum fitted by black body model at 15 million K
Excitation of D-line radiation in collisions of Na atoms with vibrationally excited N2, H2 and D2 was studied in two modulated crossed beam experiments. In both experiments, the vibrational excitation of the molecules was provided by heating the molecular beam source to temperatures in the range of 2000 to 3000 K, which was assumed to give populations according to the Boltzmann expression. In the first experiment, a total rate coefficient was measured as a function of molecular beam temperature, with absolute calibration of the photon detector being made using the black body radiation from the heated molecular beam source. Since heating affects both the internal energy and the collisional kinetic energy, the first experiment could not determine the relative contributions of internal energy transfer versus collisional excitation. The second experiment achieved partial separation of internal versus kinetic energy transfer effects by using a velocity-selected molecular beam. Using two simple models for the kinetic energy dependence of the transfer cross section for a given change in vibrational quantum number, the data from both experiments were used to determine parameters in the models.
Data on ten galactic X-ray sources were obtained during a rocket flight from Brazil in June 1969. Detailed spectra of these sources have been compared with bremsstrahlung, black body, and power law models, each including interstellar absorption. Six of the sources were fitted well by one or more of these models. In only one case were the data sufficient to distinguish the best model. Three of the sources were not fitted by any of the models, which suggests that more complex emission mechanisms are applicable. A comparison of our results with those of previous investigations provides evidence that five of the sources vary in intensity by a factor of 2 or more, and that three have variable spectra. New or substantially improved positions have been derived for four of the sources observed.