Properties of local plasma injections in Saturn's magnetosphere

By J. Burch, Jerry Goldstein, T. Hill, D. T. Young, F. Crary, A. Coates, N. André, W. Kurth, E. Sittler. 2005

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Energetic particle injections in Saturn's magnetosphere (2005, background): “Thus, injections there presumably proceed without the storage and release of magnetic energies and may be closely related to the interchange process often invoked for Jupiter [see also Burch et al., 2005; Hill et al., 2005; Thomsen et al., 2004].”
Cassini plasma spectrometer thermal ion measurements in Saturn's inner magnetosphere (2008, background): “: THERMAL IONS IN SATURN’S MAGNETOSPHERE 10 of 11 A12218 fast inward flow [Burch et al., 2005; Hill et al., 2005; Chen and Hill, 2008].”
Evidence for rotationally driven plasma transport in Saturn's magnetosphere (2005, background): “The lower limit is essentially the smallest age that passes our selection criteria; younger events are observed [Burch et al., 2005] but are indistinguishable from ‘‘spikes’’ with vertical slope.”
Flow of mass and energy in the magnetospheres of Jupiter and Saturn (2011, background): “…has been very rare [Thorne et al., 1997; Bolton et al., 1997; Kivelson et al., 1997; Frank and Paterson, 2000], but at Saturn the weaker field has allowed observation of many flux interchanges [André et al., 2005; Burch et al., 2005; Hill et al., 2005; Mauk et al., 2005; Chen and Hill, 2008].”