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Resonance maps for 3D Alfvén waves in a compressed dipole field
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dc.contributor.author | Wright, Andrew | |
dc.contributor.author | Degeling, Alexander | |
dc.contributor.author | Elsden, Thomas | |
dc.date.accessioned | 2022-03-31T14:32:00Z | |
dc.date.available | 2022-03-31T14:32:00Z | |
dc.date.issued | 2022-03-31 | |
dc.identifier | 278438319 | |
dc.identifier | aa3c9a78-02ce-40bb-b3c5-f30d971900fb | |
dc.identifier | 000777616200001 | |
dc.identifier | 85129271638 | |
dc.identifier.citation | Wright , 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/10.1029/2022JA030294 | en |
dc.identifier.issn | 2169-9402 | |
dc.identifier.other | ORCID: /0000-0002-9877-1457/work/110911900 | |
dc.identifier.other | ORCID: /0000-0002-1910-2010/work/110911973 | |
dc.identifier.uri | https://hdl.handle.net/10023/25130 | |
dc.description | Funding: 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.abstract | Resonance 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.extent | 12 | |
dc.format.extent | 2835970 | |
dc.language.iso | eng | |
dc.relation.ispartof | Journal of Geophysical Research: Space Physics | en |
dc.subject | Resonant Alfven waves | en |
dc.subject | Nonuniform medium | en |
dc.subject | Resonance Maps | en |
dc.subject | QA Mathematics | en |
dc.subject | QB Astronomy | en |
dc.subject | QC Physics | en |
dc.subject | DAS | en |
dc.subject | MCC | en |
dc.subject.lcc | QA | en |
dc.subject.lcc | QB | en |
dc.subject.lcc | QC | en |
dc.title | Resonance maps for 3D Alfvén waves in a compressed dipole field | en |
dc.type | Journal article | en |
dc.contributor.sponsor | Science & Technology Facilities Council | en |
dc.contributor.institution | University of St Andrews. Applied Mathematics | en |
dc.identifier.doi | 10.1029/2022JA030294 | |
dc.description.status | Peer reviewed | en |
dc.identifier.grantnumber | ST/N000609/1 | en |
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