Weakening of Jupiter's main auroral emission during January 2014

dc.bibliographicCitation.firstPage988
dc.bibliographicCitation.issue3
dc.bibliographicCitation.lastPage997
dc.bibliographicCitation.volume43
dc.contributor.authorBadman, S.V.
dc.contributor.authorBonfond, B.
dc.contributor.authorFujimoto, M.
dc.contributor.authorGray, R.L.
dc.contributor.authorKasaba, Y.
dc.contributor.authorKasahara, S.
dc.contributor.authorKimura, T.
dc.contributor.authorMelin, H.
dc.contributor.authorNichols, J.D.
dc.contributor.authorSteffl, A.J.
dc.contributor.authorTao, C.
dc.contributor.authorTsuchiya, F.
dc.contributor.authorYamazaki, A.
dc.contributor.authorYoneda, M.
dc.contributor.authorYoshikawa, I.
dc.contributor.authorYoshioka, K.
dc.date.accessioned2022-05-11T06:29:23Z
dc.date.available2022-05-11T06:29:23Z
dc.date.issued2016
dc.description.abstractIn January 2014 Jupiter's FUV main auroral oval decreased its emitted power by 70% and shifted equatorward by ∼1°. Intense, low-latitude features were also detected. The decrease in emitted power is attributed to a decrease in auroral current density rather than electron energy. This could be caused by a decrease in the source electron density, an order of magnitude increase in the source electron thermal energy, or a combination of these. Both can be explained either by expansion of the magnetosphere or by an increase in the inward transport of hot plasma through the middle magnetosphere and its interchange with cold flux tubes moving outward. In the latter case the hot plasma could have increased the electron temperature in the source region and produced the intense, low-latitude features, while the increased cold plasma transport rate produced the shift of the main oval.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/8946
dc.identifier.urihttps://doi.org/10.34657/7984
dc.language.isoengeng
dc.publisherHoboken, NJ : Wiley
dc.relation.doihttps://doi.org/10.1002/2015GL067366
dc.relation.essn1944-8007
dc.relation.ispartofseriesGeophysical research letters : GRL 43 (2016), Nr. 3
dc.rights.licenseCC BY 3.0 Unported
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/
dc.subjectauroraeng
dc.subjectfield-aligned currenteng
dc.subjectJupitereng
dc.subjectmagnetosphereeng
dc.subject.ddc550
dc.titleWeakening of Jupiter's main auroral emission during January 2014eng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleGeophysical research letters : GRL
tib.accessRightsopenAccesseng
wgl.contributorKISger
wgl.subjectGeowissenschaftenger
wgl.subjectPhysikger
wgl.typeZeitschriftenartikelger
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