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dc.contributor.authorMiller, D
dc.date.accessioned2019-07-12T12:08:00Z
dc.date.issued2019-07-29
dc.description.abstractThe Archontis dynamo is a rare example of an MHD dynamo within which forcing drives a dynamo where the flow and magnetic fields are almost perfectly aligned and the energies are approximately equal. In this paper, I expand upon our knowledge of the dynamo by showing that the intermediate steady states of the kinetic and magnetic energies observed by Cameron and Galloway are not a necessary feature of aligned dynamos. Furthermore, I show that the steady state into which the flow and magnetic fields eventually evolve is remarkably robust to the addition of time dependence and asymmetry to the forcing.en_GB
dc.description.sponsorshipEngineering and Physical Sciences Research Council (EPSRC)en_GB
dc.identifier.citationVol. 113 (4), pp. 405-423
dc.identifier.doi10.1080/03091929.2019.1640876
dc.identifier.grantnumber636452en_GB
dc.identifier.urihttp://hdl.handle.net/10871/37966
dc.language.isoenen_GB
dc.publisherTaylor & Francisen_GB
dc.relation.urlhttps://doi.org/10.24378/exe.1603en_GB
dc.subjectDynamo theoryen_GB
dc.subjectMHDen_GB
dc.titleEvolution of Aligned States Within Nonlinear Dynamos (article)en_GB
dc.typeArticleen_GB
dc.date.available2019-07-12T12:08:00Z
dc.identifier.issn0309-1929
dc.descriptionThis is the final version. Available on open access from Taylor & Francis via the DOI in this recorden_GB
dc.descriptionThe dataset associated with this article is located in ORE at: https://doi.org/10.24378/exe.1603en_GB
dc.identifier.journalGeophysical and Astrophysical Fluid Dynamicsen_GB
dc.rights.urihttp://www.rioxx.net/licenses/all-rights-reserveden_GB
dcterms.dateAccepted2019-07-04
rioxxterms.versionVoRen_GB
rioxxterms.licenseref.startdate2019-07-04
rioxxterms.typeJournal Article/Reviewen_GB
refterms.dateFCD2019-07-11T15:10:14Z
refterms.versionFCDAM
refterms.dateFOA2019-07-31T12:47:54Z
refterms.panelBen_GB


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