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dc.contributor.authorArregui, I
dc.contributor.authorSoler, R
dc.contributor.authorBallester, J.
dc.contributor.authorWright, Andrew Nicholas
dc.date.accessioned2014-01-16T10:31:10Z
dc.date.available2014-01-16T10:31:10Z
dc.date.issued2011-09
dc.identifier.citationArregui , I , Soler , R , Ballester , J & Wright , A N 2011 , ' Magnetohydrodynamic kink waves in two-dimensional non-uniform prominence threads ' , Astronomy & Astrophysics , vol. 533 , A60 . https://doi.org/10.1051/0004-6361/201117477en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 23150171
dc.identifier.otherPURE UUID: 79f1c43d-363b-4745-b540-de9e5057e176
dc.identifier.otherScopus: 80052148987
dc.identifier.otherORCID: /0000-0002-9877-1457/work/58055401
dc.identifier.urihttp://hdl.handle.net/10023/4374
dc.description.abstractAims. We analyse the oscillatory properties of resonantly damped transverse kink oscillations in two-dimensional prominence threads. Methods. The fine structures are modelled as cylindrically symmetric magnetic flux tubes with a dense central part with prominence plasma properties and an evacuated part, both surrounded by coronal plasma. The equilibrium density is allowed to vary non-uniformly in both the transverse and the longitudinal directions. We examine the influence of longitudinal density structuring on periods, damping times, and damping rates for transverse kink modes computed by numerically solving the linear resistive magnetohydrodynamic (MHD) equations. Results. The relevant parameters are the length of the thread and the density in the evacuated part of the tube, two quantities that are difficult to directly estimate from observations. We find that both of them strongly influence the oscillatory periods and damping times, and to a lesser extent the damping ratios. The analysis of the spatial distribution of perturbations and of the energy flux into the resonances allows us to explain the obtained damping times. Conclusions. Implications for prominence seismology, the physics of resonantly damped kink modes in two-dimensional magnetic flux tubes, and the heating of prominence plasmas are discussed.
dc.format.extent12
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights© 2011, ESO. A&A 533, A60 (2011). Reproduced with permission from the publishers.en
dc.subjectMagnetohydrodynamics (MHD)en
dc.subjectSunen
dc.subjectFilamentsen
dc.subjectProminencesen
dc.subjectWavesen
dc.subjectQB Astronomyen
dc.subject.lccQBen
dc.titleMagnetohydrodynamic kink waves in two-dimensional non-uniform prominence threadsen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201117477
dc.description.statusPeer revieweden


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