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dc.contributor.authorMiller, Daniel
dc.date.accessioned2019-07-11T14:03:40Z
dc.date.issued2019-07-10
dc.date.updated2019-07-11T13:24:53Z
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.doi10.24378/exe.1603
dc.identifier.grantnumber1636452en_GB
dc.identifier.urihttp://hdl.handle.net/10871/37958
dc.language.isoenen_GB
dc.publisherUniversity of Exeteren_GB
dc.relation.urlhttp://hdl.handle.net/10871/37966en_GB
dc.rightsCC BY 4.0en_GB
dc.subjectMHDen_GB
dc.subjectdynamosen_GB
dc.titleEvolution of Aligned States Within Nonlinear Dynamos (dataset)en_GB
dc.typeDataseten_GB
dc.date.available2019-07-11T14:03:40Z
dc.descriptionThe article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/37966en_GB
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_GB
rioxxterms.versionNAen_GB
rioxxterms.licenseref.startdate2019-07-10
rioxxterms.typeOtheren_GB
refterms.dateFOA2019-07-11T14:03:48Z


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