The results and interpretation of some of the Harvard OSO-IV observations.
OSO-4 solar UV spectrum measurements, correlating chromospheric line intensity and photospheric magnetic field strengths
Goldberg, L.↗
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Results for “interpreted”
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 interpretation of the peculiar helium star HZ 29.
Variable He star HZ29, noting unusually wide and shallow He I lines and possible mass and composition
Stothers, R.↗
Interpretation of passive current maxima during polarization of stainless steels.
Passive current maxima during anodic polarization of stainless steel in sulfuric acid, using electrochemical and electron microprobes
France, W. D., Jr.↗
Engineering models of the Venus atmosphere based on an interpretation of recent space vehicle observations of Venus.
Venusian atmosphere model developed from satellite and earth based radar data for environmental criteria in spacecraft design and mission planning
Schiffer, R. A.↗
An interpretation of OGO light ion abundance measurements.
Light ion abundance measurements of OGO satellites and field aligned diffusive equilibrium theory with temperature and concentration latitudinal variations
Colin, L.↗
On the interpretation of intensity ratios of forbidden iron and calcium transitions in the solar corona.
Intensity ratios effect of forbidden Fe and Ca transitions in solar corona on Fe/Ca ratio, noting cascading configurations
Smith, T. S.↗
Mars - Interpretation of spectral reflectivity of light and dark regions.
Spectral reflectivity curves for Mars light and dark areas and seasonal changes of dark area simulated in laboratory
Adams, J. B.↗
Meteorological interpretation of satellite radiation data Semiannual status report, 1 Oct. 1968 - 31 Mar. 1969
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Source record↗
Interpretation of wind-tunnel data in terms of dynamic behaviour of aircraft at high angles of attack
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Stone, R. W., Jr.↗
Interpretation of microwave spectral- absorption intensity measurements on partially saturated lines
Intensity measurements of microwave spectral absorption on partially saturated lines
Easley, W. C.↗
Application of structural analysis and matrix interpretive system
Computer program for matrix manipulations of structural analysis
Bamford, R. M.↗
The detector package for the lunar ranging experiment at McDonald Observatory. Supplement 2 - Interpretation of star measurements and other supplementary items
System configurations and daily star measurement
Poultney, S. K.↗
Interpretation of XUV spectroheliograms.
Chromospheric structural parameters determined from XUV spectroheliograms, discussing He 2 emission, O 4 and O 5 emission distribution, etc
Zirin, H.↗
Interpretation of lunar mass concentrations
Lunar mascon origin theories, discussing mass transfer by excess pressure generation due to rapid cooling crust and densification by water outgassing
Kaula, W. M.↗
Photometry for interpretation
Photometry as aid for aerial photography, discussing resolution, mapping, etc
Musgrove, R. G.↗
Interpretation of high-resolution spectra of Venus. I
High resolution Venus spectra, obtaining band spectra growth curve of C13O16O18 isotope of carbon dioxide, comparing data reduction methods
Young, L. G.↗
Radar maps of the moon at 70-cm wavelength and their interpretation
Polarized and depolarized radar maps of moon, attributing anomalies and average diffuse component of echoes to scattering behavior of surface and subsurface rocks
Campbell, M. J.↗
Interpretation of high-resolution spectra of Mars. I - CO2 abundance and surface pressure derived from the curve of growth
Mars carbon dioxide abundance and surface pressure from growth curve based on high resolution spectra
Young, L. D. G.↗