Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants .
Abstract not provided.
Johnston, Mark↗
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Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants .
Abstract not provided.
Johnston, Mark↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants .
Abstract not provided.
Johnston, Mark↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants .
Abstract not provided.
Johnston, Mark↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants .
Abstract not provided.
Smith, Trevor↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants
Explore the source record for details and available documents.
Schwarz, Jens↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants
Explore the source record for details and available documents.
Johnston, Mark D.↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants
Explore the source record for details and available documents.
Smith, Trevor Johannes↗
Understanding electrode plasma formation on wires and thin foils via vacuum ultraviolet spectroscopy of desorbed surface contaminants
Explore the source record for details and available documents.
Schwarz, Jens↗
Planetary ultraviolet spectroscopy.
Spaceborne planetary UV spectroscopic search for atoms and molecules basic to life, specifically molecular N and water vapor photodissociation products
Barth, C. A.↗
Far-ultraviolet spectroscopy of Jupiter
Far UV spectroscopy of Jupiter by rocket-borne spectrograph
Jenkins, E. B.↗
Ultraviolet spectroscopy experiment for Mariner Mars 1971
Scanning UV spectrometer for Mariner Mars 1971 orbital mission, investigating atmospheric composition for biological activity
Barth, C. A.↗
Minor constituents in planetary atmospheres: Ultraviolet spectroscopy from the orbiting astronomical observatory
OAO data between 2000 A and 3600 A, obtained by the Wisconsin experimental package objective grating scanning spectrometer, are used to set upper limits to the abundances of many minor constituents in the atmospheres of Mars, Jupiter, Saturn, and Venus.
Owen, T.↗
Minor constituents in planetary atmospheres - Ultraviolet spectroscopy from the Orbiting Astronomical Observatory.
Orbiting Astronomical Observatory data between 2000 and 3600 A, obtained by the Wisconsin Experimental Package objective grating scanning spectrometer, are used to set upper limits to the abundances of many minor constituents in the atmospheres of Mars, Jupiter, Saturn, and Venus.
Owen, T.↗
Outer planets Grand Tour ultraviolet spectroscopy experiment
The principal objective is presented of the UV observations, with emphasis placed on hydrogen and helium. Calculations are given for airglow and occultation. Mission requirements and trajectories are also reported for future observations.
Donahue, T. M.↗
Ultraviolet spectroscopy of binary systems
Four typical binary systems that illustrate some of the major problems in the study of binary stars are discussed. Consideration is given to (1) high-luminosity X-ray sources typified by Cyg X-1 (HDE 226868) and Vela XR-1 (HD 77581), (2) low-luminosity X-ray sources (HZ Her), (3) late-type systems of W UMa and RS CVn type, and (4) cool supergiants with a hot companion (VV Cephei).
Dupree, A. K.↗
Ultraviolet spectroscopy of comets
The UV spectra of a comet, Comet Seargent 1978m, were obtained two weeks after the comet's discovery before any ground-based spectroscopic observations were made. The second comet observed with IUE was Comet Bradfield 1979e. It was first observed on January 10 and 11, 1980, and subsequently on several occasions until the beginning of March of 1980. The comets were observed at various heliocentric distances in the low and high dispersion mode. In the long wavelength region, emission bands of OH, CS, CO2(+), NH and CO(+) were identified, and the rotational structures of the (0, 0) and (1, 0) bands of OH were resolved. In the short wavelength region, emission lines of H(L alpha), O I, C I, C II, and C 1 and the CO fourth positive bands appeared. The results of these observations are the detection of S I; indications that CS exists as "Parent Molecules" in the cometary ice; the resolution of the (0, 0) and (1, 0) bands of OH; the determination of the spatial variations of various emissions; the determination of the variation of the production rates of various species, especially of H and OH, with heliocentric distance.
Rahe, J.↗
Ultraviolet spectroscopy of comets
The advantages of the space shuttle being used as an observing platform with advanced instrumentation for the study of comets are discussed. The ground-based observations of the comet West (1976) were used to illustrate the many problems caused by the Earth's atmosphere. The spectrum of comet Bennett (1970 II) was compared to that the of comet West in order to correct instrument errors.
Lillie, C. F.↗