Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/32635
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dc.contributor.authorBelenkaya, E. S.-
dc.contributor.authorCowley, Stanley W. H.-
dc.contributor.authorMeredith, C. J.-
dc.contributor.authorNichols, J. D.-
dc.contributor.authorKalegaev, V. V.-
dc.contributor.authorAlexeev, I. I.-
dc.contributor.authorBarinov, O. G.-
dc.contributor.authorBarinova, W. O.-
dc.contributor.authorBlokhina, M. S.-
dc.date.accessioned2015-07-13T14:58:54Z-
dc.date.available2015-07-13T14:58:54Z-
dc.date.issued2014-06-27-
dc.identifier.citationAnnales Geophysicae, 2014, 32 (6), pp. 689-704 (16)en
dc.identifier.issn0992-7689-
dc.identifier.urihttp://www.ann-geophys.net/32/689/2014/angeo-32-689-2014.htmlen
dc.identifier.urihttp://hdl.handle.net/2381/32635-
dc.description.abstractA unique set of images of Saturn's northern polar UV aurora was obtained by the Hubble Space Telescope in 2011 and 2012 at times when the Cassini spacecraft was located in the solar wind just upstream of Saturn's bow shock. This rare situation provides an opportunity to use the Kronian paraboloid magnetic field model to examine source locations of the bright auroral features by mapping them along field lines into the magnetosphere, taking account of the interplanetary magnetic field (IMF) measured near simultaneously by Cassini. It is found that the persistent dawn arc maps to closed field lines in the dawn to noon sector, with an equatorward edge generally located in the inner part of the ring current, typically at ~ 7 Saturn radii (R[subscript: S]) near dawn, and a poleward edge that maps variously between the centre of the ring current and beyond its outer edge at ~ 15 R[subscript: S], depending on the latitudinal width of the arc. This location, together with a lack of response in properties to the concurrent IMF, suggests a principal connection with ring-current and nightside processes. The higher-latitude patchy auroras observed intermittently near to noon and at later local times extending towards dusk are instead found to straddle the model open–closed field boundary, thus mapping along field lines to the dayside outer magnetosphere and magnetopause. These emissions, which occur preferentially for northward IMF directions, are thus likely associated with reconnection and open-flux production at the magnetopause. One image for southward IMF also exhibits a prominent patch of very high latitude emissions extending poleward of patchy dawn arc emissions in the pre-noon sector. This is found to lie centrally within the region of open model field lines, suggesting an origin in the current system associated with lobe reconnection, similar to that observed in the terrestrial magnetosphere for northward IMF.en
dc.language.isoenen
dc.publisherCopernicus Publications on behalf of the European Geosciences Unionen
dc.rightsCopyright © the authors, 2014. This is an open-access article distributed under the terms of the Creative Commons Attribution License ( http://creativecommons.org/licenses/by/3.0/ ), 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.subjectGeosciences, Multidisciplinaryen
dc.subjectMeteorology & Atmospheric Sciencesen
dc.subjectGeologyen
dc.subjectASTRONOMY & ASTROPHYSICSen
dc.subjectGEOSCIENCES, MULTIDISCIPLINARYen
dc.subjectMETEOROLOGY & ATMOSPHERIC SCIENCESen
dc.subjectMagnetospheric physicsen
dc.subjectplanetary magnetospheresen
dc.subjectHUBBLE-SPACE-TELESCOPEen
dc.subjectIMF DEPENDENCEen
dc.subjectLINE BOUNDARYen
dc.subjectRECONNECTIONen
dc.subjectIONOSPHEREen
dc.subjectOVALen
dc.subjectMAGNETOPAUSEen
dc.subjectDYNAMICSen
dc.subjectCONVECTIONen
dc.subjectCOMPONENTen
dc.titleMagnetospheric magnetic field modelling for the 2011 and 2012 HST Saturn aurora campaigns - implications for auroral source regionsen
dc.typeJournal Articleen
dc.identifier.doi10.5194/angeo-32-689-2014-
dc.identifier.eissn1432-0576-
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.dateaccepted2014-05-20-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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