The origin of Saturn's magnetic periodicities: Northern and southern current systems

Abstract

The recent survey by Andrews et al. (2012) of the separate northern and southern ∼10.7 h periodic magnetic signals in Saturn's magnetosphere limits very much their governing current systems. The existence of signals with pure or close to pure northern or southern periods in respective polar caps taken with the relatively narrow bandwidth of the signals indicates that the actual periodicities are imposed independently from northern and southern polar regions, i.e., the open field line regions. Field-aligned currents must flow on the boundaries of these regions to exclude signals from the other hemisphere. Equatorward of the polar cap, on closed magnetic shells, there are distinct north and south "cam" source currents, the distinction being made clear by a difference in polarization. We outline the consequences for the governing current systems and the implications for sustaining the energy and power dissipation in the system. Key Points Current systems for the 10.7 h Saturnian magnetic signals are given Signal sources are in the polar caps, i.e., open field line regions The energy source is a dynamo process driven in each polar ionosphere ©2014. American Geophysical Union. All Rights Reserved.