Evidence for rotationally driven plasma transport in Saturn's magnetosphere

By Travis W. Hill, A. Rymer, J. Burch, F. Crary, D. Young, M. Thomsen, D. Delapp, N. André, A. Coates, G. Lewis. 2005

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Survey of ion plasma parameters in Saturn's magnetosphere (2010, background): “This is particularly a problem for the H+ because time‐of‐flight data (not shown) indicate that the hot injected ions [e.g., Hill et al., 2005] are predominantly composed of light ions.”
A Saturnian longitude system based on a variable kilometric radiation period (2006, background): “One might immediately think of magnetospheric phenomena such as injection events [cf. Hill et al., 2005] that might demonstrate some relationship with this system, but others may benefit from exploration using this system, as well.”
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].”
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].”
Energetic particle injections in Saturn's magnetosphere (2005, methodology): “For the dipole configuration, one may estimate Wg after Lew [1961] and Hamlin et al. [1961] for Saturn with:”