Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorReid, Jack
dc.contributor.authorParnell, Clare Elizabeth
dc.contributor.authorHood, Alan William
dc.contributor.authorBrowning, P. K.
dc.date.accessioned2019-12-02T13:30:06Z
dc.date.available2019-12-02T13:30:06Z
dc.date.issued2019-11-21
dc.identifier.citationReid , J , Parnell , C E , Hood , A W & Browning , P K 2019 , ' Determining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null points ' , Astronomy & Astrophysics . https://doi.org/10.1051/0004-6361/201936832en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 263841431
dc.identifier.otherPURE UUID: 82a139be-fe59-4a66-9535-d21b6dc49705
dc.identifier.urihttp://hdl.handle.net/10023/19041
dc.descriptionFunding: Carnegie Trust for the Universities of Scotland; Science and Technology Facilities Council (grants ST/S000402/1 and ST/P000428/1).en
dc.description.abstractThe squashing factor of a magnetic field, Q, is commonly used as an indicator of magnetic reconnection, but few studies seek to evaluate how reliable it is in comparison with other possible reconnection indicators. By using a full, self-consistent, three-dimensional, resistive magnetohydrodynamic experiment of interacting magnetic strands constituting a coronal loop, Q and several different quantities are determined. Each is then compared with the necessary and sufficient condition for reconnection, namely the integral along a field line of the component of the electric field parallel to the magnetic field. Among the reconnection indicators explored, we find the squashing factor less successful when compared with alternatives, such as Ohmic heating. In a reconnecting magnetic field devoid of null points, our work suggests that Q, being a geometric measure of the magnetic field, is not a reliable indicator of the onset or a diagnostic of the location of magnetic reconnection in some configurations.
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rightsCopyright © 2019 ESO. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the author created accepted manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://doi.org/10.1051/0004-6361/201936832en
dc.subjectSun: coronaen
dc.subjectSun: magnetic fieldsen
dc.subjectMagnetic reconnectionen
dc.subjectMagnetohydrodynamics (MHD)en
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectT-NDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleDetermining whether the squashing factor, Q, would be a good indicator of reconnection in a resistive MHD experiment devoid of null pointsen
dc.typeJournal articleen
dc.description.versionPostprinten
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201936832
dc.description.statusPeer revieweden


This item appears in the following Collection(s)

Show simple item record