Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/33193
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dc.contributor.authorJinks, S. L.-
dc.contributor.authorBunce, E. J.-
dc.contributor.authorCowley, Stanley W. H.-
dc.contributor.authorProvan, G.-
dc.contributor.authorYeoman, T. K.-
dc.contributor.authorArridge, C. S.-
dc.contributor.authorDougherty, M. K.-
dc.contributor.authorGurnett, D. A.-
dc.contributor.authorKrupp, N.-
dc.contributor.authorKurth, W. S.-
dc.contributor.authorMitchell, D. G.-
dc.contributor.authorMorooka, M.-
dc.contributor.authorWahlund, J-E.-
dc.date.accessioned2015-10-08T10:33:51Z-
dc.date.available2015-10-08T10:33:51Z-
dc.date.issued2014-10-01-
dc.identifier.citationJournal of Geophysical Research. Space Physics , 2014, 119 (10), pp. 8161-8177 (17)en
dc.identifier.issn2169-9380-
dc.identifier.urihttp://onlinelibrary.wiley.com/doi/10.1002/2014JA020367/abstracten
dc.identifier.urihttp://hdl.handle.net/2381/33193-
dc.description.abstractWe present the first systematic investigation of the polar cap boundary in Saturn's high-latitude magnetosphere through a multi-instrument assessment of various Cassini in situ data sets gathered between 2006 and 2009. We identify 48 polar cap crossings where the polar cap boundary can be clearly observed in the step in upper cutoff of auroral hiss emissions from the plasma wave data, a sudden increase in electron density, an anisotropy of energetic electrons along the magnetic field, and an increase in incidence of higher-energy electrons from the low-energy electron spectrometer measurements as we move equatorward from the pole. We determine the average level of coincidence of the polar cap boundary identified in the various in situ data sets to be 0.34° ± 0.05° colatitude. The average location of the boundary in the southern (northern) hemisphere is found to be at 15.6° (13.3°) colatitude. In both hemispheres we identify a consistent equatorward offset between the poleward edge of the auroral upward directed field-aligned current region of ~1.5–1.8° colatitude to the corresponding polar cap boundary. We identify atypical observations in the boundary region, including observations of approximately hourly periodicities in the auroral hiss emissions close to the pole. We suggest that the position of the southern polar cap boundary is somewhat ordered by the southern planetary period oscillation phase but that it cannot account for the boundary's full latitudinal variability. We find no clear evidence of any ordering of the northern polar cap boundary location with the northern planetary period magnetic field oscillation phase.en
dc.language.isoenen
dc.publisherAmerican Geophysical Union (AGU)en
dc.rightsCopyright ©2014. The Authors. This is an open access article under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.en
dc.subjectScience & Technologyen
dc.subjectPhysical Sciencesen
dc.subjectAstronomy & Astrophysicsen
dc.subjectSaturnen
dc.subjectmagnetosphereen
dc.subjectpolar capen
dc.subjecthigh latitudeen
dc.subjectMAGNETOSPHERE-IONOSPHERE SYSTEMen
dc.subjectFIELD LINE BOUNDARYen
dc.subjectSOLAR-WINDen
dc.subjectELECTRON-DENSITYen
dc.subjectMAGNETIC-FIELDen
dc.subjectAURORAL OVALen
dc.subjectFLOWSen
dc.subjectLOCATIONen
dc.subjectRECONNECTIONen
dc.subjectMAGNETOPAUSEen
dc.titleCassini multi-instrument assessment of Saturn's polar cap boundaryen
dc.typeJournal Articleen
dc.identifier.doi10.1002/2014JA020367-
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
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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