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Electrostatic solitary waves observed at Saturn by Cassini inside 10 R s and near Enceladus
Author(s) -
Pickett J. S.,
Kurth W. S.,
Gurnett D. A.,
Huff R. L.,
Faden J. B.,
Averkamp T. F.,
Píša D.,
Jones G. H.
Publication year - 2015
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
eISSN - 2169-9402
pISSN - 2169-9380
DOI - 10.1002/2015ja021305
Subject(s) - enceladus , saturn , physics , plume , amplitude , magnetosphere , plasma , astrobiology , astrophysics , optics , planet , meteorology , quantum mechanics
We have analyzed the Cassini Radio and Plasma Wave Science Wideband Receiver (WBR) data specifically looking for the presence of bipolar electrostatic solitary waves (ESWs). Typical examples of these ESWs are provided to show that when they are present, several of them may be detected over a few to several millisecond time span. We carried out an event study of an Enceladus encounter which took place on 9 October 2008. Approximately 30 min prior to and during the crossing of the Enceladus dust plume, several ESWs are observed with amplitudes of about 100 μV/m up to about 140 mV/m, and time durations of several tens of microseconds up to 250 µs. The highest amplitudes (over 10 mV/m) were observed only during the closest approach to Enceladus. We also carried out an ESW survey using the WBR for all years from 2004 to 2008 for distances less than 10 R s . The survey clearly shows that most of the ESWs are found on the nightside, with a high percentage of them in the range of 4–6 R s . This location is consistent with the densest part of Saturn's E ring and Enceladus' orbit. These are the first extended survey results of ESWs near Saturn and the first reported ESWs in connection with Enceladus. We discuss possibilities for the generation of these nonlinear ESWs, which involve current, beam, and acoustic, including dust, instabilities.