E A Marouf
Overview
Explore the profile of E A Marouf including associated specialties, affiliations and a list of published articles.
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Articles
6
Citations
19
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0
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Recent Articles
1.
Cuzzi J, Burns J, Charnoz S, Clark R, Colwell J, Dones L, et al.
Science
. 2010 Mar;
327(5972):1470-5.
PMID: 20299586
We review our understanding of Saturn's rings after nearly 6 years of observations by the Cassini spacecraft. Saturn's rings are composed mostly of water ice but also contain an undetermined...
2.
Tyler G, Sweetnam D, Anderson J, Borutzki S, Campbell J, Eshleman V, et al.
Science
. 1989 Dec;
246(4936):1466-73.
PMID: 17756001
The Voyager 2 encounter with the Neptune system included radio science investigations of the masses and densities of Neptune and Triton, the low-order gravitational harmonics of Neptune, the vertical structures...
3.
Tyler G, Sweetnam D, Anderson J, Campbell J, Eshleman V, Hinson D, et al.
Science
. 1986 Jul;
233(4759):79-84.
PMID: 17812893
Voyager 2 radio occultation measurements of the Uranian atmosphere were obtained between 2 and 7 degrees south latitude. Initial atmospheric temperature profiles extend from pressures of 10 to 900 millibars...
4.
Eshleman V, Tyler G, Simpson R, Marouf E
Science
. 1984 Feb;
223(4638):772.
PMID: 17737737
No abstract available.
5.
Esposito L, Borderies N, Goldreich P, Cuzzi J, Holberg J, Lane A, et al.
Science
. 1983 Oct;
222(4619):57-60.
PMID: 17810092
The Voyager spacecraft observed a narrow, eccentric ringlet in the Maxwell gap (1.45 Saturn radii) in Saturn's rings. Intercomparison of the Voyager imaging, photopolarimeter, ultraviolet spectrometer, and radio science observations...
6.
Marouf E, Tyler G
Science
. 1982 Jul;
217(4556):243-5.
PMID: 17814464
Classical edge diffraction patterns are formed at centimeter wavelengths by several features of Saturn's rings. These patterns were discovered in 3.6-and 13-centimeter radio signals from Voyager 1 during occultation by...