dc.contributor.author | Miller, Daniel | |
dc.date.accessioned | 2019-07-11T14:03:40Z | |
dc.date.issued | 2019-07-10 | |
dc.date.updated | 2019-07-11T13:24:53Z | |
dc.description.abstract | The 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.sponsorship | Engineering and Physical Sciences Research Council (EPSRC) | en_GB |
dc.identifier.doi | 10.24378/exe.1603 | |
dc.identifier.grantnumber | 1636452 | en_GB |
dc.identifier.uri | http://hdl.handle.net/10871/37958 | |
dc.language.iso | en | en_GB |
dc.publisher | University of Exeter | en_GB |
dc.relation.url | http://hdl.handle.net/10871/37966 | en_GB |
dc.rights | CC BY 4.0 | en_GB |
dc.subject | MHD | en_GB |
dc.subject | dynamos | en_GB |
dc.title | Evolution of Aligned States Within Nonlinear Dynamos (dataset) | en_GB |
dc.type | Dataset | en_GB |
dc.date.available | 2019-07-11T14:03:40Z | |
dc.description | The article associated with this dataset is located in ORE at: http://hdl.handle.net/10871/37966 | en_GB |
dc.rights.uri | https://creativecommons.org/licenses/by/4.0/ | en_GB |
rioxxterms.version | NA | en_GB |
rioxxterms.licenseref.startdate | 2019-07-10 | |
rioxxterms.type | Other | en_GB |
refterms.dateFOA | 2019-07-11T14:03:48Z | |