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dc.contributor.authorRachmeler, L.A.
dc.contributor.authorPlatten, S.J.
dc.contributor.authorBethge, C.
dc.contributor.authorSeaton, D.B.
dc.contributor.authorYeates, A.R.
dc.date.accessioned2014-09-02T09:31:05Z
dc.date.available2014-09-02T09:31:05Z
dc.date.issued2014-05-20
dc.identifier.citationRachmeler , L A , Platten , S J , Bethge , C , Seaton , D B & Yeates , A R 2014 , ' Observations of a hybrid double-streamer/pseudostreamer in the solar corona ' , Astrophysical Journal Letters , vol. 787 , no. 1 , L3 . https://doi.org/10.1088/2041-8205/787/1/L3en
dc.identifier.issn2041-8205
dc.identifier.otherPURE: 145263533
dc.identifier.otherPURE UUID: ea9d3b4f-37a0-485f-96bb-908d29fb07b7
dc.identifier.otherScopus: 84900401296
dc.identifier.otherWOS: 000336035800003
dc.identifier.urihttps://hdl.handle.net/10023/5318
dc.descriptionD.B.S. and L.A.R. acknowledge support from the Belgian Federal Science Policy Office (BELSPO) through the ESA-PRODEX program, grant No. 4000103240. S.J.P. acknowledges the financial support of the Isle of Man Government.en
dc.description.abstractWe report on the first observation of a single hybrid magnetic structure that contains both a pseudostreamer and a double streamer. This structure was originally observed by the SWAP instrument on board the PROBA2 satellite between 2013 May 5 and 10. It consists of a pair of filament channels near the south pole of the Sun. On the western edge of the structure, the magnetic morphology above the filaments is that of a side-by-side double streamer, with open field between the two channels. On the eastern edge, the magnetic morphology is that of a coronal pseudostreamer without the central open field. We investigated this structure with multiple observations and modeling techniques. We describe the topology and dynamic consequences of such a unified structure.
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Lettersen
dc.rights© 2014. The American Astronomical Society. All rights reserved.en
dc.subjectSun: coronaen
dc.subjectSun: filaments, prominencesen
dc.subjectSun: magnetic fieldsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleObservations of a hybrid double-streamer/pseudostreamer in the solar coronaen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.contributor.institutionUniversity of St Andrews. School of Mathematics and Statisticsen
dc.contributor.institutionUniversity of St Andrews. Pure Mathematicsen
dc.identifier.doihttps://doi.org/10.1088/2041-8205/787/1/L3
dc.description.statusPeer revieweden


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