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dc.contributor.authorE. H. Stevenson, Julie
dc.contributor.authorE. Parnell, Clare
dc.date.accessioned2016-06-09T23:32:38Z
dc.date.available2016-06-09T23:32:38Z
dc.date.issued2015-12
dc.identifier.citationE. H. Stevenson , J & E. Parnell , C 2015 , ' Spontaneous reconnection at a separator current layer : I. Nature of the reconnection ' , Journal of Geophysical Research: Space Physics , vol. 120 , no. 12 , pp. 10334-10352 . https://doi.org/10.1002/2015JA021730en
dc.identifier.issn2169-9402
dc.identifier.otherPURE: 225630555
dc.identifier.otherPURE UUID: 8f1ddba5-4c44-4cba-97ed-410fd6f56d36
dc.identifier.otherArXiv: http://arxiv.org/abs/1509.07729v2
dc.identifier.otherScopus: 84956932603
dc.identifier.otherORCID: /0000-0002-5694-9069/work/73700740
dc.identifier.otherWOS: 000369180200015
dc.identifier.urihttp://hdl.handle.net/10023/8959
dc.description.abstractMagnetic separators, which lie on the boundary between four topologically-distinct flux domains, are prime locations in three-dimensional magnetic fields for reconnection, especially in the magnetosphere between the planetary and interplanetary magnetic fields and also in the solar atmosphere. Little is known about the details of separator reconnection and so the aim of this paper, which is the first of two, is to study the properties of magnetic reconnection at a single separator. Three-dimensional, resistive magnetohydrodynamic numerical experiments are run to study separator reconnection starting from a magnetohydrostatic equilibrium which contains a twisted current layer along a single separator linking a pair of opposite-polarity null points. The resulting reconnection occurs in two phases. The first is short involving rapid reconnection in which the current at the separator is reduced by a factor of around 2.3. Most 75% of the magnetic energy is converted during this phase, via Ohmic dissipation, directly into internal energy, with just 0.1% going into kinetic energy. During this phase the reconnection occurs along most of the separator away from its ends (the nulls), but in an asymmetric manner which changes both spatially and temporally over time. The second phase is much longer and involves slow impulsive-bursty reconnection. Again Ohmic heating dominates over viscous damping. Here the reconnection occurs in small localized bursts at random anywhere along the separator.
dc.format.extent19
dc.language.isoeng
dc.relation.ispartofJournal of Geophysical Research: Space Physicsen
dc.rights© 2015, Publisher / the Author(s). This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at onlinelibrary.wiley.com / https://dx.doi.org/10.1002/2015JA021736en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subjectBDCen
dc.subjectR2Cen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleSpontaneous reconnection at a separator current layer : I. Nature of the reconnectionen
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.identifier.doihttps://doi.org/10.1002/2015JA021730
dc.description.statusPeer revieweden
dc.date.embargoedUntil2016-06-10


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