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The interaction of the atmosphere of Enceladus with Saturn's plasma.

Authors :
Tokar RL
Johnson RE
Hill TW
Pontius DH
Kurth WS
Crary FJ
Young DT
Thomsen MF
Reisenfeld DB
Coates AJ
Lewis GR
Sittler EC
Gurnett DA
Source :
Science (New York, N.Y.) [Science] 2006 Mar 10; Vol. 311 (5766), pp. 1409-12.
Publication Year :
2006

Abstract

During the 14 July 2005 encounter of Cassini with Enceladus, the Cassini Plasma Spectrometer measured strong deflections in the corotating ion flow, commencing at least 27 Enceladus radii (27 x 252.1 kilometers) from Enceladus. The Cassini Radio and Plasma Wave Science instrument inferred little plasma density increase near Enceladus. These data are consistent with ion formation via charge exchange and pickup by Saturn's magnetic field. The charge exchange occurs between neutrals in the Enceladus atmosphere and corotating ions in Saturn's inner magnetosphere. Pickup ions are observed near Enceladus, and a total mass loading rate of about 100 kilograms per second (3 x 10(27) H(2)O molecules per second) is inferred.

Details

Language :
English
ISSN :
1095-9203
Volume :
311
Issue :
5766
Database :
MEDLINE
Journal :
Science (New York, N.Y.)
Publication Type :
Academic Journal
Accession number :
16527967
Full Text :
https://doi.org/10.1126/science.1121061