Search Results - (Author, Cooperation:R. A. West)
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1Latest Papers from Table of Contents or Articles in PressE. P. Turtle ; J. E. Perry ; A. G. Hayes ; R. D. Lorenz ; J. W. Barnes ; A. S. McEwen ; R. A. West ; A. D. Del Genio ; J. M. Barbara ; J. I. Lunine ; E. L. Schaller ; T. L. Ray ; R. M. Lopes ; E. R. Stofan
American Association for the Advancement of Science (AAAS)
Published 2011Staff ViewPublication Date: 2011-03-19Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsKeywords: Atmosphere ; Extraterrestrial Environment ; *Methane ; *Saturn ; SpacecraftPublished by: -
2Latest Papers from Table of Contents or Articles in PressLiming Li; X. Jiang; R. A. West; P. J. Gierasch; S. Perez-Hoyos; A. Sanchez-Lavega; L. N. Fletcher; J. J. Fortney; B. Knowles; C. C. Porco; K. H. Baines; P. M. Fry; A. Mallama; R. K. Achterberg; A. A. Simon; C. A. Nixon; G. S. Orton; U. A. Dyudina; S. P. Ewald; R. W. Schmude Jr.
Nature Publishing Group (NPG)
Published 2018Staff ViewPublication Date: 2018-09-14Publisher: Nature Publishing Group (NPG)Electronic ISSN: 2041-1723Topics: BiologyChemistry and PharmacologyNatural Sciences in GeneralPhysicsPublished by: -
3Latest Papers from Table of Contents or Articles in PressStaff View
Publication Date: 2018-06-21Publisher: Royal SocietyElectronic ISSN: 2054-5703Topics: Natural Sciences in GeneralKeywords: organic chemistry, synthetic chemistryPublished by: -
4Articles: DFG German National LicensesBrown, M. E. ; Salinas, S. V. ; Bouchez, A. H. ; Roe, H. G. ; West, R. A.
[s.l.] : Nature Publishing Group
Published 2005Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] With its substantial atmosphere of nitrogen, hydrocarbons and nitriles, Saturn's moon Titan is a unique planetary satellite. Photochemical processing of the gaseous constituents produces an extended haze that obscures the surface. Soon after the Voyager fly-bys in 1980 and 1981 ...Type of Medium: Electronic ResourceURL: -
5Articles: DFG German National LicensesStaff View
ISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] THE following particulars of the circumstances attending a lightning flash are perhaps worth recording. A cedar tree (deodar) 50 feet high stood at a distance considerably less than its own height from a house at Englefield Green. The lddy of the house was sitting watching the storm, but ...Type of Medium: Electronic ResourceURL: -
6Articles: DFG German National LicensesHord, C. W. ; McClintock, W. E. ; Stewart, A. I. F. ; Barth, C. A. ; Esposito, L. W. ; Thomas, G. E. ; Sandel, B. R. ; Hunten, D. M. ; Broadfoot, A. L. ; Shemansky, D. E. ; Ajello, J. M. ; Lane, A. L. ; West, R. A.
Springer
Published 1992Staff ViewISSN: 1572-9672Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract The Galileo ultraviolet spectrometer experiment uses data obtained by the Ultraviolet Spectrometer (UVS) mounted on the pointed orbiter scan platform and from the Extreme Ultraviolet Spectrometer (EUVS) mounted on the spinning part of the orbiter with the field of view perpendicular to the spin axis. The UVS is a Ebert-Fastie design that covers the range 113–432 nm with a wavelength resolution of 0.7 nm below 190 and 1.3 nm at longer wavelengths. The UVS spatial resolution is 0.4 deg × 0.1 deg for illuminated disc observations and 1 deg × 0.1 deg for limb geometries. The EUVS is a Voyager design objective grating spectrometer, modified to cover the wavelength range from 54 to 128 nm with wavelength resolution 3.5 nm for extended sources and 1.5 nm for point sources and spatial resolution of 0.87 deg × 0.17 deg. The EUVS instrument will follow up on the many Voyager UVS discoveries, particularly the sulfur and oxygen ion emissions in the Io torus and molecular and atomic hydrogen auroral and airglow emissions from Jupiter. The UVS will obtain spectra of emission, absorption, and scattering features in the unexplored, by spacecraft, 170–432 nm wavelength region. The UVS and EUVS instruments will provide a powerful instrument complement to investigate volatile escape and surface composition of the Galilean satellites, the Io plasma torus, micro- and macro-properties of the Jupiter clouds, and the composition structure and evolution of the Jupiter upper atmosphere.Type of Medium: Electronic ResourceURL: