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Volumn 327, Issue 5972, 2010, Pages 1470-1475

An evolving view of saturn's dynamic rings

(23)  Cuzzi, J N a   Burns, J A b   Charnoz, S c   Clark, R N d   Colwell, J E e   Dones, L f   Esposito, L W g   Filacchione, G h   French, R G i   Hedman, M M b   Kempf, S j   Marouf, E A k   Murray, C D l   Nicholson, P D b   Porco, C C m   Schmidt, J n   Showalter, M R o   Spilker, L J p   Spitale, J N m   Srama, R j   more..

c DIF   (France)

Author keywords

[No Author keywords available]

Indexed keywords

GRAVITY; SATURN; SOLAR SYSTEM; SPACECRAFT;

EID: 77949797334     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1179118     Document Type: Review
Times cited : (103)

References (78)
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    • 2 dr, where n(r) is the vertically integrated number density per radius increment for particles of radius r, and we have assumed that the ring particles are much larger than the wavelength of light. For small number densities, this is effectively the projected surface area of particles per unit ring area. Usually this is expressed as the "normal" optical depth, corresponding to rays arriving perpendicular to the mean plane of the rings.
    • 2 dr, where n(r) is the vertically integrated number density per radius increment for particles of radius r, and we have assumed that the ring particles are much larger than the wavelength of light. For small number densities, this is effectively the projected surface area of particles per unit ring area. Usually this is expressed as the "normal" optical depth, corresponding to rays arriving perpendicular to the mean plane of the rings.
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    • We applaud with gratitude the Cassini spacecraft engineering and operations teams. We thank the other members of the Cassini Rings Discipline Working group for their many contributions, not all of which could be described here. We thank our Ring Science Planning Team leaders at JPL-B.
    • We applaud with gratitude the Cassini spacecraft engineering and operations teams. We thank the other members of the Cassini Rings Discipline Working group for their many contributions, not all of which could be described here. We thank our Ring Science Planning Team leaders at JPL-B.
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    • R. E. Johnson, R. Pappalardo, P. Kalas, C. Niebur for helpful suggestions on presentation. The U.S. authors were supported by NASA through the Cassini Project and Cassini Data Analysis Program. Other support was provided by the Italian Space Agency (ASI), Deutsches Zentrum für Luft und Raumfahrt (DLR), the Newton Institute, Université Paris Diderot and CEA-Saclay, and the U.K. Science and Technology Facilities Council.
    • R. E. Johnson, R. Pappalardo, P. Kalas, and C. Niebur for helpful suggestions on presentation. The U.S. authors were supported by NASA through the Cassini Project and Cassini Data Analysis Program. Other support was provided by the Italian Space Agency (ASI), Deutsches Zentrum für Luft und Raumfahrt (DLR), the Newton Institute, Université Paris Diderot and CEA-Saclay, and the U.K. Science and Technology Facilities Council.


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