Spectral-Line Profiles for a Fast-Ion-Beam Source
Exact expression for line profile of stigmatic spectrograph without vignetting, noting results with foil-excited ions as light source
SPECTRAL LINE WIDTH↗
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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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Ultraviolet reflectivity of Venus and Jupiter.
Rocketborne spectrograph measurement of UV REFLECTIVITY of Venus and Jupiter, noting atmospheric Rayleigh scattering effects
ROCKET SOUNDING↗
Far ultra-violet spectra of Orion stars.
Far UV spectra of brighter stars in vicinity of epsilon Orionis photographed with objective spectrograph carried by rocket
STELLAR SPECTRUM↗
Nitric acid-organic mixtures surveyed for use in separation by anion exchange methods
Column elution-spectrographic analysis technique compares certain solvents directly to the methanol system, using inert rare earths instead of actinides. Distribution ratios for americium between 90 percent solvent, 10 percent 5 M nitric acid and Dowex 1 nitrate form resin for a large group of organics miscible in water was determined.
Bloomquist, C. A. A.↗
Development of chemical analysis techniques for advanced materials Quarterly progress report, 17 Jul. - 16 Oct. 1967
Chemical analysis of hydroxyl in solid magnesium oxide using chemical decomposition and emission and mass spectrographic techniques
Blosser, E. R.↗
Development of chemical analysis techniques for advanced materials Quarterly progress report, 17 Jan. - 16 Apr. 1968
Laser decomposition, hydroxyl determination, and mass spectrographic studies in magnesium oxide/ graphite/hydroxyl systems
Blosser, E. R.↗
On the binary nature of Cyg X-2.
Cyg X-2 X ray source binary nature observed from spectrogram using prime focus spectrograph and solid Schmidt camera
Burbidge, E. M.↗
Explosive high-speed shutter.
Explosive high speed spectrographic shutter noting opening, closing, triggering and delay times
Nims, D. J.↗
Comparison of selected carbon stars and M stars at 1 micron.
Spectrographic comparison of selected carbon and M stars, discussing atomic lines identifications
Fay, T. D.↗
The absorption-line spectrum of the quasi- stellar object PHL 5200.
Quasar PHL 5200 absorption line spectrum from prime focus spectrograph on Lick 120 inch telescope in November 1967, noting Si IV absorption lines
Burbidge, E. M.↗
Mass spectograph analysis
Computer program provides a means of rapid data reduction of mass spectrograph data. The methods used are suited to mechanization on a digital computer since they consist of the systematic search of a large amount of tabular data and the unknown.
Shores, J. P.↗
Ultraviolet stellar astronomy, Experiment S019 Final report, 27 Aug. 1965 - 31 Dec. 1967
Wide angle objective prism spectrograph for ultraviolet stellar astronomy
Wackerling, L. R.↗
Solar cell contact development Quarterly report, 28 Jun. - 28 Sep. 1968
Auger spectrographic analysis on titanium-silver contact degradation in silicon solar cells
Source record↗
A high-resolution study of the C super 3 pi sub 1 goes to B super 3 pi sub g /0,0/ stimulated transitions in N sub 2.
High resolution spectroscopic study of stimulated rotational transitions of nitrogen molecules using crossed grating Echelle spectrograph
Javan, A.↗
General review of beam-foil spectroscopy.
Beam-foil spectroscopy problems noting light collection, spectrograph design, broadening of spectral lines by Doppler effect and other complications
Bashkin, S.↗
Far-ultraviolet spectra of zeta Puppis and gamma super 2 Velorum.
Far UV spectra of zeta Puppis and gamma super two Velorum with 1.6 A resolution photographed with all reflective objective spectrograph on Aerobee rocket
Brooks, N. H.↗
Absorption spectrum of electrically excited oxygen molecules. II.
Absorption spectrum of diatomic oxygen excited by AC silent discharge photographed with vacuum spectrograph, associating lines with Schumann- Runge band
Chang, H.-C.↗
Nitric acid vapor above 19 km in the earth's atmosphere.
Nitric acid vapor in atmosphere as function of altitude from spectrograph, predicting downward diffusion
Rhine, P. E.↗