Jupiter's South Equatorial Belt cycle in 2009-2011: II, The SEB Revival
John H. Rogers

TL;DR
This paper details the 2010-2011 revival of Jupiter's South Equatorial Belt, highlighting the sequence of large-scale disturbances, plume formations, and convective activity, validated by detailed observations and consistent with historical descriptions.
Contribution
It provides a comprehensive observational analysis of Jupiter's SEB revival, identifying key features and mechanisms, and confirms that these phenomena follow a typical pattern observed in past events.
Findings
The revival began with a bright white plume from a cyclonic oval.
Multiple high-altitude methane-bright plumes appeared along the outbreak track.
The central outbreak consisted of large convective cells initiated by bright plumes.
Abstract
A Revival of the South Equatorial Belt (SEB) is an organised disturbance on a grand scale. It starts with a single vigorous outbreak from which energetic storms and disturbances spread around the planet in the different zonal currents. The Revival that began in 2010 was better observed than any before it. The observations largely validate the historical descriptions of these events: the major features portrayed therein, albeit at lower resolution, are indeed the large structural features described here. Our major conclusions about the 2010 SEB Revival are as follows, and we show that most of them may be typical of SEB Revivals. 1) The Revival started with a bright white plume. 2) The initial plume erupted in a pre-existing cyclonic oval ('barge'). Subsequent white plumes continued to appear on the track of this barge, which was the location of the sub-surface source of the whole…
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Taxonomy
TopicsAstro and Planetary Science · Geology and Paleoclimatology Research · Geomagnetism and Paleomagnetism Studies
