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dc.contributor.authorReid, Jack
dc.contributor.authorHood, Alan William
dc.contributor.authorParnell, Clare Elizabeth
dc.contributor.authorBrowning, P. K.
dc.contributor.authorCargill, Peter
dc.date.accessioned2020-01-17T10:30:08Z
dc.date.available2020-01-17T10:30:08Z
dc.date.issued2018-07-18
dc.identifier.citationReid , J , Hood , A W , Parnell , C E , Browning , P K & Cargill , P 2018 , ' Coronal energy release by MHD avalanches : continuous driving ' , Astronomy & Astrophysics , vol. 615 , 84 . https://doi.org/10.1051/0004-6361/201732399en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 252750837
dc.identifier.otherPURE UUID: c0ab03bb-51ac-4e19-a64a-02db5672274b
dc.identifier.otherWOS: 000439524600001
dc.identifier.otherWOS: 000439524600001
dc.identifier.otherORCID: /0000-0003-2620-2068/work/58055172
dc.identifier.otherScopus: 85064343830
dc.identifier.otherORCID: /0000-0002-6391-346X/work/63716887
dc.identifier.otherORCID: /0000-0002-5694-9069/work/73700733
dc.identifier.urihttp://hdl.handle.net/10023/19299
dc.descriptionFunding: Carnegie Trust for the Universities of Scotland; Science and Technology Facilities Council (grants ST/N000609/1 and ST/P000428/1).en
dc.description.abstractPrevious work has confirmed the concept of a magnetohydrodynamic (MHD) avalanche in pre-stressed threads within a coronal loop. We undertook a series of full, three-dimensional MHD simulations in order to create three threads by twisting the magnetic field through boundary motions until an instability ensues. We find that, following the original instability, one unstable thread can disrupt its neighbours with continued driving. A ‘bursty’ heating profile results, with a series of ongoing energy releases, but no evident steady state. For the first time using full MHD, we show that avalanches are a viable mechanism for the storing and release of magnetic energy in the solar corona, as a result of photospheric motions.
dc.format.extent10
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights© 2018, ESO. This work has been made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at https://doi.org/10.1051/0004-6361/201732399en
dc.subjectSun: coronaen
dc.subjectSun: magnetic fieldsen
dc.subjectMagnetohydrodynamic (MHD)en
dc.subjectMethods: numericalen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleCoronal energy release by MHD avalanches : continuous drivingen
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/10.1051/0004-6361/201732399
dc.description.statusPeer revieweden


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