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dc.contributor.authorMacTaggart, David
dc.contributor.authorHood, Alan William
dc.date.accessioned2014-05-09T09:31:00Z
dc.date.available2014-05-09T09:31:00Z
dc.date.issued2010-06-04
dc.identifier.citationMacTaggart , D & Hood , A W 2010 , ' Simulating the "Sliding Doors" Effect Through Magnetic Flux Emergence ' , Astrophysical Journal Letters , vol. 716 , no. 2 , pp. L219-L222 . https://doi.org/10.1088/2041-8205/716/2/L219en
dc.identifier.issn2041-8205
dc.identifier.otherPURE: 4157302
dc.identifier.otherPURE UUID: 96db817d-79aa-486d-8ad4-fc9fa4d169a5
dc.identifier.otherScopus: 84859948473
dc.identifier.otherORCID: /0000-0003-2620-2068/work/58055182
dc.identifier.urihttps://hdl.handle.net/10023/4742
dc.descriptionD.M. acknowledges financial assistance from STFC. The computational work for this Letter was carried out on the joint STFC and SFC (SRIF) funded cluster at the University of St. Andrews. D.M. and A.W.H. acknowledge financial support form the European Commission through the SOLAIRE Network (MTRN-CT-2006-035484).en
dc.description.abstractRecent Hinode photospheric vector magnetogram observations have shown that the opposite polarities of a long arcade structure move apart and then come together. In addition to this "sliding doors" effect, orientations of horizontal magnetic fields along the polarity inversion line on the photosphere evolve from a normal-polarity configuration to an inverse one. To explain this behavior, a simple model by Okamoto et al. suggested that it is the result of the emergence of a twisted flux rope. Here, we model this scenario using a three-dimensional megnatohydrodynamic simulation of a twisted flux rope emerging into a pre-existing overlying arcade. We construct magnetograms from the simulation and compare them with the observations. The model produces the two signatures mentioned above. However, the cause of the "sliding doors" effect differs from the previous model.
dc.format.extent4
dc.language.isoeng
dc.relation.ispartofAstrophysical Journal Lettersen
dc.rights© 2010. The American Astronomical Society. All rights reserved.en
dc.subjectMagnetohydrodynamics (MHD)en
dc.subjectSun: photosphereen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleSimulating the "Sliding Doors" Effect Through Magnetic Flux Emergenceen
dc.typeJournal articleen
dc.contributor.sponsorPPARC - Now STFCen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1088/2041-8205/716/2/L219
dc.description.statusPeer revieweden
dc.identifier.grantnumberPP/E001122/1en


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