{"id":{"repo_id":"cape-town","oai_identifier":"oai:open.uct.ac.za:11427/28929"},"canonical_url":"https://search.dev.ndltd.org/etd/cape-town/oai:open.uct.ac.za:11427/28929","repository":{"repo_id":"cape-town","name":"University of Cape Town","base_url":"https://open.uct.ac.za/oai/request"},"display":{"title":"On the study of analogues in cosmic magnetism","abstract":"The dynamo process, by which the strength of the magnetic field is amplified, is still not well understood and, in part, requires an understanding of the behaviour of the plasma fluid (i.e. a charged fluid) in different conditions. It has long been known that charged and non-charged fluids display similar behaviour to each other, with key quantities such as the magnetic field, B, and fluid vorticity, ω, being both structurally-similar and playing similar roles to each other in their respective evolution equations.","abstract_html":"The dynamo process, by which the strength of the magnetic field is amplified, is still not well understood and, in part, requires an understanding of the behaviour of the plasma fluid (i.e. a charged fluid) in different conditions. It has long been known that charged and non-charged fluids display similar behaviour to each other, with key quantities such as the magnetic field, B, and fluid vorticity, ω, being both structurally-similar and playing similar roles to each other in their respective evolution equations.","abstract_has_math":false,"creators":["Adams, Patrick William"],"institution":"Department of Statistical Sciences","degree_name":null,"degree_level":null,"degree_discipline":null,"degree_department":null,"school":null,"contributors":[],"advisors":["Osano, B"],"committee_chairs":[],"committee_members":[],"year":2017,"date_issued":"2017","date_published":"2017","updated_at":"2026-07-22T22:23:16Z","subjects":[],"languages":["eng"],"rights":[],"rights_urls":[],"identifier_entries":[]},"links":{"outbound_url":"http://hdl.handle.net/11427/28929","outbound_label":"Handle","outbound_source":"dc:identifier.uri"},"metadata_groups":[{"id":"people","label":"People","entries":[{"key":"dc:contributor.advisor","label":"Advisor","values":["Osano, B"]},{"key":"dc:creator","label":"Author","values":["Adams, Patrick William"]}]},{"id":"academic_context","label":"Academic Context","entries":[{"key":"dc:date.accessioned","label":"Dc Date Accessioned","values":["2018-10-17T10:34:09Z"]},{"key":"dc:date.available","label":"Dc Date Available","values":["2018-10-17T10:34:09Z"]},{"key":"dc:date.issued","label":"Date","values":["2017"]},{"key":"dc:publisher.department","label":"Dc Publisher Department","values":["Department of Statistical Sciences"]},{"key":"dc:publisher.institution","label":"Dc Publisher Institution","values":["University of Cape Town"]},{"key":"dc:type","label":"Dc Type","values":["Doctoral Thesis"]},{"key":"dc:type.qualificationlevel","label":"Dc Type Qualificationlevel","values":["Doctoral"]},{"key":"dc:type.qualificationname","label":"Dc Type Qualificationname","values":["PhD"]}]},{"id":"language_rights","label":"Language and Rights","entries":[{"key":"dc:language","label":"Dc Language","values":["eng"]}]},{"id":"identifiers","label":"Identifiers","entries":[{"key":"dc:identifier.uri","label":"Identifier URI","values":["http://hdl.handle.net/11427/28929"]}]},{"id":"additional","label":"Additional Metadata","entries":[{"key":"dc:description.abstract","label":"Abstract","values":["The dynamo process, by which the strength of the magnetic field is amplified, is still not well understood and, in part, requires an understanding of the behaviour of the plasma fluid (i.e. a charged fluid) in different conditions. It has long been known that charged and non-charged fluids display similar behaviour to each other, with key quantities such as the magnetic field, B, and fluid vorticity, ω, being both structurally-similar and playing similar roles to each other in their respective evolution equations."]},{"key":"dc:title","label":"Title","values":["On the study of analogues in cosmic magnetism"]}]}],"canonical_facts":{"dc:contributor.advisor":["Osano, B"],"dc:creator":["Adams, Patrick William"],"dc:date.accessioned":["2018-10-17T10:34:09Z"],"dc:date.available":["2018-10-17T10:34:09Z"],"dc:date.issued":["2017"],"dc:description.abstract":["The dynamo process, by which the strength of the magnetic field is amplified, is still not well understood and, in part, requires an understanding of the behaviour of the plasma fluid (i.e. a charged fluid) in different conditions. 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