Search Results - (Author, Cooperation:P. Edenhofer)
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1W. Kofman ; A. Herique ; Y. Barbin ; J. P. Barriot ; V. Ciarletti ; S. Clifford ; P. Edenhofer ; C. Elachi ; C. Eyraud ; J. P. Goutail ; E. Heggy ; L. Jorda ; J. Lasue ; A. C. Levasseur-Regourd ; E. Nielsen ; P. Pasquero ; F. Preusker ; P. Puget ; D. Plettemeier ; Y. Rogez ; H. Sierks ; C. Statz ; H. Svedhem ; I. Williams ; S. Zine ; J. Van Zyl
American Association for the Advancement of Science (AAAS)
Published 2015Staff ViewPublication Date: 2015-08-01Publisher: American Association for the Advancement of Science (AAAS)Print ISSN: 0036-8075Electronic ISSN: 1095-9203Topics: BiologyChemistry and PharmacologyComputer ScienceMedicineNatural Sciences in GeneralPhysicsPublished by: -
2Allison, M. ; Asmar, S. W. ; Atkinson, D. H. ; Avruch, I. M. ; Dutta-Roy, R. ; Dzierma, Y. ; Edenhofer, P. ; Folkner, W. M. ; Gurvits, L. I. ; Johnston, D. V. ; Plettemeier, D. ; Pogrebenko, S. V. ; Preston, R. A. ; Tyler, G. L. ; Bird, M. K.
[s.l.] : Nature Publishing Group
Published 2005Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] One of Titan's most intriguing attributes is its copious but featureless atmosphere. The Voyager 1 fly-by and occultation in 1980 provided the first radial survey of Titan's atmospheric pressure and temperature and evidence for the presence of strong zonal winds. It was realized that ...Type of Medium: Electronic ResourceURL: -
3Bird, M.K. ; Asmar, S.W. ; Edenhofer, P. ; Funke, O. ; Patzold, M. ; Volland, H.
Amsterdam : ElsevierStaff ViewISSN: 0032-0633Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: GeosciencesPhysicsType of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 0273-1177Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision MechanicsPhysicsType of Medium: Electronic ResourceURL: -
5Staff View
ISSN: 0273-1177Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: Mechanical Engineering, Materials Science, Production Engineering, Mining and Metallurgy, Traffic Engineering, Precision MechanicsPhysicsType of Medium: Electronic ResourceURL: -
6Edenhofer, P. ; Bird, M. K. ; Brenkle, J. P. ; Buschert, H. ; Esposito, P. B. ; Porsche, H. ; Volland, H.
[s.l.] : Nature Publishing Group
Published 1986Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] The scientific objectives of the Giotto Radio-Science Experiment (GRE) are to determine the columnar electron content of comet Halley's ionosphere and the mass fluence of the cometary atmosphere1'2. For this purpose the radio signals from the Giotto spacecraft were used during the Halley encounter ...Type of Medium: Electronic ResourceURL: -
7Howard, H. T. ; Eshleman, V. R. ; Hinson, D. P. ; Kliore, A. J. ; Lindal, G. F. ; Woo, R. ; Bird, M. K. ; Volland, H. ; Edenhofer, P. ; Pätzold, M. ; Porsche, H.
Springer
Published 1992Staff ViewISSN: 1572-9672Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract The radio science investigations planned for Galileo's 6-year flight to and 2-year orbit of Jupiter use as their instrument the dual-frequency radio system on the spacecraft operating in conjunction with various US and German tracking stations on Earth. The planned radio propagation experiments are based on measurements of absolute and differential propagation time delay, differential phase delay, Doppler shift, signal strength, and polarization. These measurements will be used to study: the atmospheric and ionospheric structure, constituents, and dynamics of Jupiter; the magnetic field of Jupiter; the diameter of Io, its ionospheric structure, and the distribution of plasma in the Io torus; the diameters of the other Galilean satellites, certain properties of their surfaces, and possibly their atmospheres and ionospheres; and the plasma dynamics and magnetic field of the solar corona. The spacecraft system used for these investigations is based on Voyager heritage but with several important additions and modifications that provide linear rather than circular polarization on the S-band downlink signal, the capability to receive X-band uplink signals, and a differential downlink ranging mode. Collaboration between the investigators and the space-craft communications engineers has resulted in the first highly-stable, dual-frequency, spacecraft radio system suitable for simultaneous measurements of all the parameters normally attributed to radio waves.Type of Medium: Electronic ResourceURL: