Planetary Period Modulation of Reconnection Bursts in Saturn's Magnetotail. Issue 11 (28th November 2018)

• Record Type: Journal Article
• Authors: Bradley, T. J.; Cowley, S. W. H.; Bunce, E. J.; Smith, A. W.; Jackman, C. M.; Provan, G.
• Is Part Of: Journal of geophysical research. Volume 123:Issue 11(2018)
• Page Start: 9476
• Page End: 9507
• Publication Date: 2018-11-28
• Subjects: magnetic reconnection -- PPO -- Saturn -- magnetotail -- dipolarization -- plasmoid; Magnetospheric physics -- Periodicals; Space environment -- Periodicals; Cosmic physics -- Periodicals; Planets -- Atmospheres -- Periodicals; Heliosphere (Astrophysics) -- Periodicals; Geophysics -- Periodicals; 523.01
• DOI: 10.1029/2018JA025932
• Languages: English
• ISSNs: 2169-9380

Abstract

Abstract: We conduct a statistical analysis of 2, 094 reconnection events in Saturn's near‐equatorial magnetotail previously identified in Cassini magnetometer data from intervals during 2006 and 2009/2010. These consist of tailward propagating plasmoids and planetward propagating dipolarizations, with approximately twice as many plasmoids as dipolarizations. We organize these by three related planetary period oscillation (PPO) phase systems, the northern and southern PPO phases relative to noon, the same phases retarded by a radial propagation delay, and the local retarded phases that take account of the azimuth (local time) of the observation. Clear PPO modulation is found for both plasmoid and dipolarization events, with local retarded phases best organizing the event data with the modulation in event frequency propagating across the tail as the PPO systems rotate. This indicates that the events are localized in azimuth, rather than simultaneously affecting much of the tail width. Overall, events occur preferentially by factors of ~3 at northern and southern phases where the tail current sheet is expected locally to be thinnest in the PPO cycle, with field lines contracting back from their maximum radial displacement, compared with the antiphase conditions. Separating the events into those representing the start of independent reconnection episodes, occurring at least 3 hr after the last, and events in subsequent clusters, shows that the above phases are predominantly characteristic of the majority cluster events. The phases at the start of independent reconnection episodes are typically ~60° earlier. Key Points: We analyze a catalogue of 2, 094 reconnection events in Saturn's magnetotail and organize them according to northern and southern PPO phases Events are best organized by local PPO phases rather than global phases, implying that reconnection is more locally than globally triggered Events are best organized by phases where the tail current sheet should be locally thin and the field lines near maximum radial displacement