Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36240
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dc.contributor.authorNichols, Jonathan D.-
dc.contributor.authorBadman, S. V.-
dc.contributor.authorBunce, E. J.-
dc.contributor.authorClarke, J. T.-
dc.contributor.authorCowley, Stanley William Herbert-
dc.contributor.authorHunt, G. J.-
dc.contributor.authorProvan, G.-
dc.date.accessioned2016-01-11T09:53:44Z-
dc.date.available2016-01-11T09:53:44Z-
dc.date.issued2016-01-01-
dc.identifier.citationIcarus, 2016, 263, pp. 17-31 (15)en
dc.identifier.issn0019-1035-
dc.identifier.urihttp://www.sciencedirect.com/science/article/pii/S001910351500411Xen
dc.identifier.urihttp://hdl.handle.net/2381/36240-
dc.description.abstractWe discuss the features of Saturn’s northern FUV auroras as observed during a program of Hubble Space Telescope observations which executed over 2011–2013 and culminated, along with Cassini observations, in a comprehensive multi-spectral observing campaign. Our 2011–2013 observations of the northern aurora are also compared with those from our 2007–2008 observation of the southern aurora. We show that the variety of morphologies of the northern auroras is broadly consistent with the southern, and determine the statistical equatorward and poleward boundary locations. We find that our boundaries are overall consistent with previous observations, although a modest poleward displacement of the poleward boundaries is due to the increased prevalence of poleward auroral patches in the noon and afternoon sectors during this program, likely due to the solar wind interaction. We also show that the northern auroral oval oscillates with the northern planetary period oscillation (PPO) phase in an elongated ellipse with semi-major axis ∼1.6° oriented along the post-dawn/post-dusk direction. We further show that the northern auroras exhibit dawn-side brightenings at zero northern magnetic PPO phase, although there is mixed evidence of auroral emissions fixed in the rotating frame of the northern PPO current system, such that overall the dependence of the auroras on northern magnetic phase is somewhat weak.en
dc.language.isoenen
dc.publisherElsevier for Academic Press Inc.en
dc.rightsCopyright © 2015, the Authors. Published by Elsevier Inc. This is an open access article under the CC BY license ( http://creativecommons.org/licenses/by/4.0/ ) which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.en
dc.subjectScience & Technologyen
dc.subjectPhysical Sciencesen
dc.subjectAstronomy & Astrophysicsen
dc.subjectSaturnen
dc.subjectMagnetospheresen
dc.subjectAuroraeen
dc.subjectHubble Space Telescope observationsen
dc.subjectINTERPLANETARY MAGNETIC-FIELDen
dc.subjectULTRAVIOLET AURORAen
dc.subjectMAGNETOSPHEREen
dc.subjectCUSPen
dc.titleSaturn's northern auroras as observed using the Hubble Space Telescopeen
dc.typeJournal Articleen
dc.identifier.doi10.1016/j.icarus.2015.09.008-
dc.description.statusPeer-revieweden
dc.description.versionPublisher Versionen
dc.type.subtypeArticle;Journal-
pubs.organisational-group/Organisationen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERINGen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomyen
dc.dateaccepted2015-09-04-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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