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dc.contributor.authorMcLaughlin, James Alexander
dc.contributor.authorDe Moortel, Ineke
dc.contributor.authorHood, Alan William
dc.date.accessioned2014-01-14T13:01:08Z
dc.date.available2014-01-14T13:01:08Z
dc.date.issued2011-02
dc.identifier.citationMcLaughlin , J A , De Moortel , I & Hood , A W 2011 , ' Phase mixing of nonlinear visco-resistive Alfvén waves ' , Astronomy & Astrophysics , vol. 527 , A149 . https://doi.org/10.1051/0004-6361/201015552en
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 13753935
dc.identifier.otherPURE UUID: f9fb255a-4ffc-4bf2-9d73-fce9ae6746b1
dc.identifier.otherScopus: 79951634598
dc.identifier.otherORCID: /0000-0002-1452-9330/work/39526480
dc.identifier.otherORCID: /0000-0003-2620-2068/work/58055226
dc.identifier.urihttps://hdl.handle.net/10023/4367
dc.description.abstractAims: We investigate the behaviour of nonlinear, nonideal Alfvén wave propagation within an inhomogeneous magnetic environment. Methods: The governing MHD equations are solved in 1D and 2D using both analytical techniques and numerical simulations. Results: We find clear evidence for the ponderomotive effect and visco-resistive heating. The ponderomotive effect generates a longitudinal component to the transverse Alfvén wave, with a frequency twice that of the driving frequency. Analytical work shows the addition of resistive heating. This leads to a substantial increase in the local temperature and thus gas pressure of the plasma, resulting in material being pushed along the magnetic field. In 2D, our system exhibits phase mixing and we observe an evolution in the location of the maximum heating, i.e. we find a drifting of the heating layer. Conclusions: Considering Alfvén wave propagation in 2D with an inhomogeneous density gradient, we find that the equilibrium density profile is significantly modified by both the flow of density due to visco-resistive heating and the nonlinear response to the localised heating through phase mixing.
dc.format.extent16
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysicsen
dc.rights© 2011, ESO. A&A 527, A149 (2011). Reproduced with permission from the publishers.en
dc.subjectMagnetohydrodynamics (MHD)en
dc.subjectMagnetic fieldsen
dc.subjectWavesen
dc.subjectShock wavesen
dc.subjectCoronaen
dc.subjectOscillationsen
dc.titlePhase mixing of nonlinear visco-resistive Alfvén wavesen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doihttps://doi.org/10.1051/0004-6361/201015552
dc.description.statusPeer revieweden


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