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dc.contributor.authorStevenson, Julie Elizabeth Helen
dc.contributor.authorParnell, Clare Elizabeth
dc.contributor.authorPriest, Eric Ronald
dc.contributor.authorHaynes, Andrew Lewis
dc.date.accessioned2014-11-18T11:31:02Z
dc.date.available2014-11-18T11:31:02Z
dc.date.issued2015-01
dc.identifier157155878
dc.identifier52d47b0f-0a2d-4bb4-826b-d6f6f26a6354
dc.identifier84918564476
dc.identifier000346901300040
dc.identifier.citationStevenson , J E H , Parnell , C E , Priest , E R & Haynes , A L 2015 , ' The nature of separator current layers in MHS equilibria I. Current parallel to the separator ' , Astronomy & Astrophysics , vol. 573 , A44 . https://doi.org/10.1051/0004-6361/201424348en
dc.identifier.issn0004-6361
dc.identifier.otherArXiv: http://arxiv.org/abs/1410.8691v1
dc.identifier.otherORCID: /0000-0002-5694-9069/work/73700725
dc.identifier.otherORCID: /0000-0003-3621-6690/work/74117724
dc.identifier.urihttps://hdl.handle.net/10023/5785
dc.descriptionJEHS would like to thank STFC for financial support during her Ph.D and CEP acknowledges support from the STFC consolidated grant.en
dc.description.abstractSeparators, which are in many ways the three-dimensional equivalent to two-dimensional nulls, are important sites for magnetic reconnection. Magnetic reconnection occurs in strong current layers which have very short length scales. The aim of this work is to explore the nature of current layers around separators. A separator is a special field line which lies along the intersection of two separatrix surfaces and forms the boundary between four topologically distinct flux domains. In particular, here the current layer about a separator that joins two 3D nulls and lies along the intersection of their separatrix surfaces is investigated. A magnetic configuration containing a single separator embedded in a uniform plasma with a uniform electric current parallel to the separator is considered. This initial magnetic setup, which is not in equilibrium, relaxes in a non-resistive manner to form an equilibrium. The relaxation is achieved using the 3D MHD code, Lare3d, with resistivity set to zero. A series of experiments with varying initial current are run to investigate the characteristics of the resulting current layers present in the final (quasi-) equilibrium states. In each experiment, the separator collapses and a current layer forms along it. The dimensions and strength of the current layer increase with initial current. It is found that separator current layers formed from current parallel to the separator are twisted. Also the collapse of the separator is a process that evolves like an infinite-time singularity where the length, width and peak current in the layer grow slowly whilst the depth of the current layer decreases.
dc.format.extent15
dc.format.extent565439
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.subjectMagnetohydrodynamics (MHD)en
dc.subject3D nullsen
dc.subjectSeparatorsen
dc.subjectCurrent layeren
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectQA Mathematicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.subject.lccQAen
dc.titleThe nature of separator current layers in MHS equilibria I. Current parallel to the separatoren
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.contributor.institutionUniversity of St Andrews. School of Mathematics and Statisticsen
dc.identifier.doi10.1051/0004-6361/201424348
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/K000950/1en


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