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Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope
Journal article   Open access   Peer reviewed

Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope

J D Nichols, S V Badman, K H Baines, R H Brown, E J Bunce, J T Clarke, S W H Cowley, F J Crary, M K Dougherty, J-C Gérard, …
Geophysical research letters, Vol.41(10), pp.3323-3330
05/28/2014
DOI: 10.1002/2014GL060186
PMCID: PMC4459195
PMID: 26074636
url
https://doi.org/10.1002/2014GL060186View
Published (Version of record) Open Access

Abstract

We present observations of significant dynamics within two UV auroral storms observed on Saturn using the Hubble Space Telescope in April/May 2013. Specifically, we discuss bursts of auroral emission observed at the poleward boundary of a solar wind-induced auroral storm, propagating at ∼330% rigid corotation from near ∼01 h LT toward ∼08 h LT. We suggest that these are indicative of ongoing, bursty reconnection of lobe flux in the magnetotail, providing strong evidence that Saturn's auroral storms are caused by large-scale flux closure. We also discuss the later evolution of a similar storm and show that the emission maps to the trailing region of an energetic neutral atom enhancement. We thus identify the auroral form with the upward field-aligned continuity currents flowing into the associated partial ring current.
Research Letters

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