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dc.contributor.authorHood, Alan William
dc.contributor.authorRuderman, Michael
dc.contributor.authorPascoe, David James
dc.contributor.authorDe Moortel, Ineke
dc.contributor.authorTerradas, Jaume
dc.contributor.authorWright, Andrew Nicholas
dc.date.accessioned2013-02-07T12:34:45Z
dc.date.available2013-02-07T12:34:45Z
dc.date.issued2013-03
dc.identifier.citationHood , A W , Ruderman , M , Pascoe , D J , De Moortel , I , Terradas , J & Wright , A N 2013 , ' Damping of kink waves by mode coupling : I. Analytical treatment ' , Astronomy & Astrophysics , vol. 551 , A39 . https://doi.org/10.1051/0004-6361/201220617en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 34921682
dc.identifier.otherPURE UUID: ba1e0950-ced0-430d-9f19-6f56799c2427
dc.identifier.otherScopus: 84874067196
dc.identifier.otherWOS: 000316460600039
dc.identifier.otherORCID: /0000-0002-1452-9330/work/39526490
dc.identifier.otherORCID: /0000-0003-2620-2068/work/58055206
dc.identifier.otherORCID: /0000-0002-9877-1457/work/58055403
dc.identifier.urihttps://hdl.handle.net/10023/3340
dc.description.abstractAims. To investigate the spatial damping of propagating kink waves in an inhomogeneous plasma. In the limit of a thin tube surrounded by a thin transition layer, an analytical formulation for kink waves driven in from the bottom boundary of the corona is presented. Methods. The spatial form for the damping of the kink mode was investigated using various analytical approximations. When the density ratio between the internal density and the external density is not too large, a simple di.erential-integral equation was used. Approximate analytical solutions to this equation are presented. Results. For the first time, the form of the spatial damping of the kink mode is shown analytically to be Gaussian in nature near the driven boundary. For several wavelengths, the amplitude of the kink mode is proportional to (1 + exp(-z2 /L2 g))/2, where L2g = 16/ǫκ2 k2 . Although the actual value of 16 in Lg depends on the particular form of the driver, this form is very general and its dependence on the other parameters does not change. For large distances, the damping profile appears to be roughly linear exponential decay. This is shown analytically by a series expansion when the inhomogeneous layer width is small enough.
dc.format.extent14
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights(c) ESO 2013en
dc.subjectMagnetohydrodynamics (MHD)en
dc.subjectSun: atmosphereen
dc.subjectSun: magnetic topologyen
dc.subjectSun: oscillationsen
dc.subjectWavesen
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleDamping of kink waves by mode coupling : I. Analytical treatmenten
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.sponsorThe Royal Societyen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201220617
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/K000950/1en
dc.identifier.grantnumbern/aen


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