On the cause of Saturn's plasma periodicity

André, N.; Coates, A. J.; Dougherty, M. K.; Young, D. T.; Mokashi, P.; Burch, J. L.; Goldstein, J.; Lewis, W. S.; Paty, C.

United States, United Kingdom, Netherlands

Abstract

Periodic plasma enhancements are examined for all Cassini orbits from December 29, 2005 through September 7, 2006. The events, which have UT durations of 3-4 hours, are centered near SLS3 longitude 10° at radial distances near 15 RS and at larger W longitudes at larger distances, reaching 180°W by 49 RS. Magnetic-field data within the events and outside 30 to 35 RS show signatures of neutral-sheet crossings and magnetic reconnection (i.e., plasmoids). We conclude that plasmoids move outward from 30-35 RS along a spiral path that rotates with the planet. The duration of these events is similar to that of SKR events, and they are ordered in the SKR-based SLS3 longitude system. A conceptual model, in which the plasmoids are triggered in the pre-midnight quadrant following (with a predictable delay) the appearance of SKR at the magnetopause and then propagate outward in a rotating spiral pattern, can explain the connection among periodicities observed in Saturn's charged particles, magnetic fields, and kilometric radiation.

2008 Geophysical Research Letters
Cassini 26