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Dynamic auroral storms on Saturn as observed by the Hubble Space Telescope..pdf (3.98 MB)

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

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journal contribution
posted on 2015-09-22, 10:49 authored by Jonathan D. Nichols, S. V. Badman, K. H. Baines, R. H. Brown, E. J. Bunce, J. T. Clarke, S. W. Cowley, F. J. Crary, M. K. Dougherty, J. C. Gérard, A. Grocott, D. Grodent, W. S. Kurth, H. Melin, D. G. Mitchell, W. R. Pryor, T. S. Stallard
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.

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Citation

Geophysical Research Letters, 2014, 41 (10), pp. 3323-3330

Author affiliation

/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy

Version

  • VoR (Version of Record)

Published in

Geophysical Research Letters

Publisher

American Geophysical Union (AGU)

issn

0094-8276

eissn

1944-8007

Acceptance date

2014-04-28

Copyright date

2014

Available date

2015-09-22

Publisher version

http://onlinelibrary.wiley.com/doi/10.1002/2014GL060186/abstract

Language

en

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