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dc.contributor.authorYardley, S. L.
dc.contributor.authorGreen, L. M.
dc.contributor.authorDriel-Gesztelyi, L. Van
dc.contributor.authorWilliams, D. R.
dc.contributor.authorMackay, D. H.
dc.date.accessioned2018-10-09T10:30:08Z
dc.date.available2018-10-09T10:30:08Z
dc.date.issued2018-10-10
dc.identifier.citationYardley , S L , Green , L M , Driel-Gesztelyi , L V , Williams , D R & Mackay , D H 2018 , ' The role of flux cancellation in eruptions from bipolar ARs ' , Astrophysical Journal , vol. 866 , no. 1 , 8 . https://doi.org/10.3847/1538-4357/aade4aen
dc.identifier.issn0004-637X
dc.identifier.otherPURE: 256147716
dc.identifier.otherPURE UUID: 101ede03-93cc-4a5d-9014-ccea5fe26ee5
dc.identifier.otherArXiv: http://arxiv.org/abs/1808.10635v1
dc.identifier.otherScopus: 85055189830
dc.identifier.otherORCID: /0000-0001-6065-8531/work/58055433
dc.identifier.otherWOS: 000446752400008
dc.identifier.urihttp://hdl.handle.net/10023/16173
dc.description.abstractThe physical processes or trigger mechanisms that lead to the eruption of coronal mass ejections (CMEs), the largest eruptive phenomenon in the heliosphere, are still undetermined. Low-altitude magnetic reconnection associated with flux cancellation appears to play an important role in CME occurrence as it can form an eruptive configuration and reduce the magnetic flux that contributes to the overlying, stabilizing field. We conduct the first comprehensive study of 20 small bipolar ARs (ARs) in order to probe the role of flux cancellation as an eruption trigger mechanism. We categorize eruptions from the bipolar regions into three types related to location, and find that the type of eruption produced depends on the evolutionary stage of the AR. In addition, we find that ARs that form eruptive structures by flux cancellation (low-altitude reconnection) had, on average, lower flux cancellation rates than the AR sample as a whole. Therefore, while flux cancellation plays a key role, by itself it is insufficient for the production of an eruption. The results provide supporting evidence that although flux cancellation in a sheared arcade may be able to build an eruptive configuration, a successful eruption depends upon the removal of sufficient overlying and stabilizing field. Convergence of the bipole polarities also appears to be present in regions that produce an eruption. These findings have important implications for understanding the physical processes that occur on our Sun in relation to CMEs and for space weather forecasting.
dc.format.extent11
dc.language.isoeng
dc.relation.ispartofAstrophysical Journalen
dc.rights© 2018, The American Astronomical Society. 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/10.3847/1538-4357/aade4aen
dc.subjectSun: activityen
dc.subjectSun: coronaen
dc.subjectSun: coronal mass ejections (CMEs)en
dc.subjectSun: evolutionen
dc.subjectSun: magnetic fielden
dc.subjectSun: photosphereen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subject3rd-DASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleThe role of flux cancellation in eruptions from bipolar ARsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.3847/1538-4357/aade4a
dc.description.statusPeer revieweden


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