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dc.contributor.authorWright, Andrew
dc.contributor.authorDegeling, Alexander
dc.contributor.authorElsden, Thomas
dc.date.accessioned2022-03-31T14:32:00Z
dc.date.available2022-03-31T14:32:00Z
dc.date.issued2022-03-31
dc.identifier278438319
dc.identifieraa3c9a78-02ce-40bb-b3c5-f30d971900fb
dc.identifier000777616200001
dc.identifier85129271638
dc.identifier.citationWright , A , Degeling , A & Elsden , T 2022 , ' Resonance maps for 3D Alfvén waves in a compressed dipole field ' , Journal of Geophysical Research: Space Physics , vol. 127 , no. 4 , e2022JA030294 . https://doi.org/10.1029/2022JA030294en
dc.identifier.issn2169-9402
dc.identifier.otherORCID: /0000-0002-9877-1457/work/110911900
dc.identifier.otherORCID: /0000-0002-1910-2010/work/110911973
dc.identifier.urihttps://hdl.handle.net/10023/25130
dc.descriptionFunding: Science and Technology Facilities Council (Grant Number(s): ST/N000609/1); National Natural Science Foundation of China (Grant Number(s): 41774172); Leverhulme Trust (Grant Number(s): ECF-2019-155).en
dc.description.abstractResonance Maps depict the possible locations and polarisations of resonant Alfvén waves (Field Line Resonances – FLRs) for a given equilibrium and driving frequency. Previously the use of Resonance Maps has been developed for gaining insight into the behavior of Alfvén waves in basic potential magnetic fields that allow the use of an orthogonal field aligned coordinate system. In more general magnetic fields these coordinates do not exist. In this paper we explore the application of Resonance Maps to such equilibria. A number of simulations of resonant Alfvén waves are presented and interpreted using the Maps. We find that Resonance Maps remain useful when some of the constructions used previously are generalised to accommodate the properties of more general magnetic fields. For example, Resonance Maps are able to predict the location and polarisation of Alfvén waves which are driven strongly by fast mode waves using a “tangential alignment condition”. Unusual properties, such as Alfvén waves crossing flux surfaces persist in the more general magnetic fields we consider.
dc.format.extent12
dc.format.extent2835970
dc.language.isoeng
dc.relation.ispartofJournal of Geophysical Research: Space Physicsen
dc.subjectResonant Alfven wavesen
dc.subjectNonuniform mediumen
dc.subjectResonance Mapsen
dc.subjectQA Mathematicsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectDASen
dc.subjectMCCen
dc.subject.lccQAen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleResonance maps for 3D Alfvén waves in a compressed dipole fielden
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. Applied Mathematicsen
dc.identifier.doi10.1029/2022JA030294
dc.description.statusPeer revieweden
dc.identifier.grantnumberST/N000609/1en


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