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dc.contributor.authorWright, Andrew
dc.contributor.authorElsden, Thomas
dc.contributor.authorDegeling, Alexander
dc.contributor.authorMann, Ian R.
dc.contributor.authorOzeke, Louis
dc.contributor.authorYeoman, Timothy
dc.contributor.authorSandhu, Jasmine
dc.contributor.authorTakahashi, Kazue
dc.date.accessioned2025-02-17T12:30:29Z
dc.date.available2025-02-17T12:30:29Z
dc.date.issued2025-02-16
dc.identifier314439192
dc.identifier51821109-6994-4b1f-b3ad-04d491165f81
dc.identifier.citationWright , A , Elsden , T , Degeling , A , Mann , I R , Ozeke , L , Yeoman , T , Sandhu , J & Takahashi , K 2025 , ' Poloidal field line resonances driven by a fast wave ' , Geophysical Research Letters , vol. 52 , no. 3 , e2024GL111670 . https://doi.org/10.1029/2024GL111670en
dc.identifier.issn0094-8276
dc.identifier.otherORCID: /0000-0002-1910-2010/work/178723804
dc.identifier.otherORCID: /0000-0002-9877-1457/work/178724035
dc.identifier.urihttps://hdl.handle.net/10023/31402
dc.descriptionThis research was supported by the International Space Science Institute (ISSI) in Bern, through ISSI International Team project #483 (The Identification and Classification of 3D Alfvén Resonances). The authors are grateful to ISSI for funding the Team and hosting its meetings. ANW was partially funded by the Science and Technology Facilities Council (STFC) Grant (ST/N000609/1). KT was supported by NASA 80NSSC19K0259. JKS was funded by STFC Grant ST/W00089X/1. AWD is funded by NSFC (RFIS-III Grant 42350710200). TKY acknowledges support from STFC UKRI Grant ST/W00089X/1 and NERC UKRI Grant NE/V000748/1. LO and IRM were supported by funding from the Canadian Space Agency. IRM was also funded by a Discovery Grant from the Canadian NSERC.en
dc.description.abstractWe present numerical simulations of the excitation of resonant poloidal Alfvén waves. The resulting Alfvén waves could be loosely described as “high‐m” (m is the azimuthal wave number) in as much as the azimuthal scale of the wave is much less than the scale in the direction normal to L‐shells. Such waves are generally excited by wave‐particle interactions. In this article we show how resonant poloidal Alfvén waves can be excited by a fast mode (of large azimuthal scale) in a cold plasma. The key property that enables this is a three‐dimensional equilibrium, which facilitates the process of phasemixing in the azimuthal direction. We show that the classification of resonant Alfvén waves as high‐m and low‐m has limited applicability in 3D inhomogeneous media and suggest an alternative classification be based on the excitation mechanism.
dc.format.extent9
dc.format.extent3391945
dc.language.isoeng
dc.relation.ispartofGeophysical Research Lettersen
dc.rights© 2025. The Author(s). This is an open access article under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits use, distribution and reproduction in any medium, provided the original work is properly cited.en
dc.subjectField line resonanceen
dc.subjectMHD wave couplingen
dc.subjectMCCen
dc.titlePoloidal field line resonances driven by a fast waveen
dc.typeJournal itemen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews.Applied Mathematicsen
dc.identifier.doi10.1029/2024GL111670
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/N000609/1en


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