Search Results - (Author, Cooperation:C. Elachi)
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1Staff View
Publication Date: 2018-01-31Publisher: Wiley-BlackwellPrint ISSN: 0148-0227Topics: GeosciencesPhysicsPublished by: -
2W. 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: -
3Janssen, M. ; Thorne, R. ; Levin, S. ; Klein, M. ; Gulkis, S. ; Bastian, T. ; Sault, R. ; Elachi, C. ; Hofstadter, M. ; Bunker, A. ; Dulk, G. ; Gudim, E. ; Hamilton, G. ; Johnson, W. T. K. ; Leblanc, Y. ; Liepack, O. ; McLeod, R. ; Roller, J. ; Roth, L. ; West, R. ; Bolton, S. J.
[s.l.] : Macmillian Magazines Ltd.
Published 2002Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Ground-based observations have shown that Jupiter is a two-component source of microwave radio emission: thermal atmospheric emission and synchrotron emission from energetic electrons spiralling in Jupiter's magnetic field. Later in situ measurements confirmed the existence of Jupiter's ...Type of Medium: Electronic ResourceURL: -
4Staff View
ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
5Staff View
ISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
6Arvidson, R.E. ; Schulte, M. ; Kwok, R. ; Curlander, J. ; Elachi, C. ; Ford, J.P. ; Saunders, R.S.
Amsterdam : ElsevierStaff ViewISSN: 0019-1035Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
7Staff View
ISSN: 0030-4018Source: Elsevier Journal Backfiles on ScienceDirect 1907 - 2002Topics: PhysicsType of Medium: Electronic ResourceURL: -
8Staff 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: -
9Staff View
ISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract The Apollo 17 ALSE VHF radar provided imagery and continuous profiling data around the Moon during two revolutions. The imagery data are used to derive depth and diameter measurements of small craters (diameter 〈30 km). The profiling data are used to study the topography of a few large craters: the bulged floors in Hevelius, Neper, and Aitken; central peaks in Neper and Buisson; and the depressed floor of Maraldi. The same data provided accurate (better than 25 m) profiles of Mare Crisium and Mare Serenitatis.Type of Medium: Electronic ResourceURL: -
10Staff View
ISSN: 1432-0649Keywords: 02 ; 41 ; 42.82Source: Springer Online Journal Archives 1860-2000Topics: PhysicsNotes: Abstract The radiation pattern of a line source lying along the plane interface of two dielectric half-spaces is calculated. It is found that the pattern at the interface has a null (interface extinction); that the pattern in the upper half-space, whose index of refraction is taken to be less than that of the lower half-space, has a single lobe with a maximum normal to the interface; and that the pattern in the lower half-space (subsurface region) has two maxima (peaks) straddling symmetrically a minimum. Interpretation of these results in terms of ray optics, Oseen's extinction theorem, and the Cerenkov effect are given.Type of Medium: Electronic ResourceURL: -
11Elachi, C. ; Lunine, J. I. ; Lorenz, R. D. ; Stiles, B. ; Mitchell, K. L. ; Ostro, S. ; Soderblom, L. ; Wood, C. ; Zebker, H. ; Wall, S. ; Janssen, M. ; Kirk, R. ; Lopes, R. ; Paganelli, F. ; Radebaugh, J. ; Wye, L. ; Anderson, Y. ; Allison, M. ; Boehmer, R. ; Callahan, P. ; Encrenaz, P. ; Flamini, E. ; Francescetti, G. ; Gim, Y. ; Hamilton, G.
[s.l.] : Nature Publishing Group
Published 2007Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] The surface of Saturn’s haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface. Initial visible and radar imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing ...Type of Medium: Electronic ResourceURL: -
12Elachi, C. ; Janssen, M. ; Stofan, E. ; Lopes, R. ; Kirk, R. ; Lorenz, R. ; Lunine, J. ; Paganelli, F. ; Soderblom, L. ; Wood, C. ; Wye, L. ; Zebker, H. ; Anderson, Y. ; Ostro, S. ; Allison, M. ; Boehmer, R. ; Callahan, P. ; Encrenaz, P. ; Flamini, E. ; Francescetti, G. ; Gim, Y. ; Hamilton, G. ; Hensley, S. ; Johnson, W. ; Kelleher, K.
[s.l.] : Nature Publishing Group
Published 2006Staff ViewISSN: 1476-4687Source: Nature Archives 1869 - 2009Topics: BiologyChemistry and PharmacologyMedicineNatural Sciences in GeneralPhysicsNotes: [Auszug] Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of ...Type of Medium: Electronic ResourceURL: -
13Campbell, W. J. ; Wayenberg, J. ; Ramseyer, J. B. ; Ramseier, R. O. ; Vant, M. R. ; Weaver, R. ; Redmond, A. ; Arsenaul, L. ; Gloersen, P. ; Zwally, H. J. ; Wilheit, T. T. ; Chang, T. C. ; Hall, D. ; Gray, L. ; Meeks, D. C. ; Bryan, M. L. ; Barath, F. T. ; Elachi, C. ; Leberl, F. ; Farr, T.
Springer
Published 1978Staff ViewISSN: 1573-1472Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract During the AIDJEX Main Experiment, April 1975 through May 1976, a comprehensive microwave sensing program was performed on the sea ice of the Beaufort Sea. Surface and aircraft measurements were obtained during all seasons using a wide variety of active and passive microwave sensors. The surface program obtained passive microwave measurements of various ice types using four antennas mounted on a tracked vehicle. In three test regions, each with an area of approximately 1.5 × 104 m2, detailed ice crystallographic, dielectric properties, and brightness temperatures of first-year, multiyear, and first-year/multiyear mixtures were measured. A NASA aircraft obtained passive microwave measurements of the entire area of the AIDJEX manned station array (triangle) during each of 18 flights. This verified the earlier reported ability to distinguish first-year and multiyear ice types and concentration and gave new information on ways to observe ice mixtures and thin ice types. The active microwave measurements from aircraft included those from an X- and L-band radar and from a scatterometer. The former is used to study a wide variety of ice features and to estimate deformations, while both are equally usable to observe ice types. With the present data, only the scatterometer can be used to distinguish positively multiyear from first-year and various types of thin ice. This is best done using coupled active and passive microwave sensing.Type of Medium: Electronic ResourceURL: -
14Staff View
ISSN: 1573-0794Source: Springer Online Journal Archives 1860-2000Topics: GeosciencesPhysicsNotes: Abstract Lunar position differences between thirteen lunar craters in Mare Serenitatis were computed from VHF radar-imagery obtained by the Lunar Sounder instrument flown on the Apollo 17 Command Module. The radar-derived position differences agree with those obtained by conventional photogrammetric reductions of Apollo metric photography. This demonstrates the feasibility of using the Apollo Lunar Sounder data to determine the positions of lunar features along the Apollo 17 orbital tracks. This will be particularly useful for western limb and farside areas, where no Apollo metric camera pictures are available.Type of Medium: Electronic ResourceURL: