Evaluation of gamma probe shielding verification for the Gemini and Apollo vehicles
Gamma probe analysis of radiation shielding for Apollo and Gemini spacecraft
Hardy, A. C.↗
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Results for “Radiation Analysis”
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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Analysis of a synthetic aperture radiating interferometer navigation satellite concept Interim technical report
Synthetic aperture interferometer navigation satellite concept
Klein, P. I.↗
Application of Monte Carlo to heat transfer problems.
Monte Carlo method application to heat transfer analysis including radiation, rarefied gas energy transfer and conduction
Howell, J. R.↗
Analysis of lateral conduction and radiation along two parallel long plates.
Lateral heat conduction and radiation along two parallel long plates separated by nonabsorbing dielectric with refractive index of unity
Armaly, B. F.↗
Flight data analysis of power subsystem degradation at near synchronous altitude Final report
Comparison and analysis of radiation damage to power supplies of satellites at near-synchronous altitudes
Picciano, W. T.↗
Refutation of Bigg's evidence for new Jovian satellites
Jovian decametric radiation periodicities analysis refuting evidence of Bigg for new Jovian satellites
Bozyan, F. A.↗
On the properties of umbral dots
Sunspot umbral dot models characteristics based on three dimensional radiative transfer analysis
Wilson, P. R.↗
Low energy cosmic rays in the solar system
Low energy cosmic radiation spectrum analysis for IMP 4 data on solar system
Kinsey, J. H.↗
The radiant heat flux limit of bypass flow in a uranium plasma rocket
Two dimensional radiative-convective analysis of bypass flow in uranium plasma rocket
Kascak, A. F.↗
Lunar surface electromagnetic sounding - A theoretical analysis
Lunar surface electromagnetic sounding, presenting analysis of radiation fields and polarization characteristics for magnetic dipole situated on layered half space
Dey, A.↗
A review of computational techniques for analysing the transfer of radiation through a model cloudy atmosphere
Model cloudy atmosphere construction, reviewing computational techniques for radiative transfer analysis
Hunt, G. E.↗
The radiation balance of the earth-atmosphere system during June and July 1969 from Nimbus 3 radiation measurements - Some preliminary results
Earth atmosphere radiation fields analysis from Nimbus 3 five-channel scanning radiometer measurements, determining mean planetary albedo and temperature
Bandeen, W. R.↗
Forecasting of the performance of MOS device for space applications
Analysis of radiation damage of MOSFET data from Explorer 34 (IMP-F), and radiation damage characteristics of MOSFET with boron diffused between a silicon semiconductor and silicon oxide are considered. The first subject is an interpretation of the discrepancy between the space data and the laboratory data. The second subject is an attempt to analyze the radiation damage characteristic of MOSFET when there is modification of electrical properties in the gate oxide region.
Fang, P. H.↗
Analysis of the Jovian electron radiation belts. II - Observations of the decimetric radiation.
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Beard, D. B.↗
Improved space radiation shielding methods
The computing software that was used to perform the charged particle radiation transport analysis and shielding design for the Mariner Jupiter/Saturn 1977 spacecraft is described. Electron fluences, energy spectra and dose rates obtained with this software are presented and compared with independent computer calculations.
Davis, H. S.↗
Evaluation of electrostatic charge effects on the data processing system and the orbiter communication and tracking receivers
An analysis of radiated interference test results obtained from frictionally charged Orbiter TPS tile was presented. The tests included the measurement of noise pick-up by Orbiter S-band, L-band, C-band, and Ku-band antennas located beneath the tiles in a manner simulating their installation on Orbiter. In addition, the radiated field characteristics resulting from the static discharge was determined. The results are analyzed as to their effect on data bus equipment and on Orbiter Communications and Tracking (C&T) receivers. It was concluded that the radiated interference should have no effect on MDM's. However the CPU, IOP and PMU enclosures require some minor modification to assure immunity from P-static interference. Orbiter antenna tests indicate that the S-band receiver should not be affected by P-static noise. The TACAN and Radar Altimeter performance appears to be adequate but with a small margin. MSBLS performance is uncertain because laboratory instrumentation cannot approach the MSBLS sensitivity.
Lawton, R. M.↗
The thermal structure of Jupiter. II - Observations and analysis of 8-14 micron radiation
Observations of Jovian limb structure at 8.11 and 8.45 microns are reported. These are used along with other limb structure and spectral data in the 8-14 micron region to derive a model of the thermal and cloud structure within the 1.0-0.01 bar pressure regime. The temperature is about 165 K at 1.00 bar, 108 K at 0.10 bar, and 143 K at 0.03 bar. In zones, an optically opaque cloud of NH3 exists near the 143 K (0.60 bar) level. A partly transparent haze of solid NH3 particles overlies the cloud. Belts are free of the cloud and have a much lower abundance of NH3 haze than the zones. The data are consistent with an NH3 gas abundance defined by saturation equilibrium, with a mixing ratio of 0.00015 deep in the atmosphere, and with a CH4 mixing ratio of 0.002, about three times the currently accepted value.
Orton, G. S.↗
Planetary spectra for anisotropic scattering
Some effects on planetary spectra that would be produced by departures from isotropic scattering are examined. The phase function is the simplest departure to handle analytically and the only phase function, other than the isotropic one, that can be incorporated into a Chandrasekhar first approximation. This approach has the advantage of illustrating effects resulting from anisotropies while retaining the simplicity that yields analytic solutions. The curve of growth is the sine qua non of planetary spectroscopy. The discussion emphasizes the difficulties and importance of ascertaining curves of growth as functions of observing geometry. A plea is made to observers to analyze their empirical curves of growth, whenever it seems feasible, in terms of coefficients of which are the leading terms in radiative-transfer analysis. An algebraic solution to the two sets of anisotropic H functions is developed which gives emergent intensities accurate to 0.3%.
Chamberlain, J. W.↗