Static and Alfvénic Electrodynamics in the Auroral Region

dc.contributor.advisorKnudsen, David J.
dc.contributor.authorWu, Jiashu
dc.contributor.committeememberBrown, Jo C.
dc.contributor.committeememberSpanswick, Emma L.
dc.contributor.committeememberDavidsen, Jörn
dc.contributor.committeememberLynch, Kristina A.
dc.contributor.committeememberPotter, Mike E.
dc.date2020-11
dc.date.accessioned2020-07-22T15:50:10Z
dc.date.available2020-07-22T15:50:10Z
dc.date.issued2020-07-21
dc.description.abstractAuroral arcs, a type of aurora with curtain-like structure, can remain quasi-static for tens of minutes, and can also appear with rapid motions and changing brightness. One of the main challenges in constructing a self-consistent theory to explain the generation and morphology of auroral arcs is an adequate description of the arc circuit, meaning the electric field and currents that span the region from the magnetospheric generator to the ionospheric footprint. The ionospheric electrodynamics plays a critical role in formation of auroral arcs and in the whole magnetosphere-ionosphere coupling system. The high-precision magnetic and electric field data collected by the Swarm satellites are well suited to study both quasi-static auroral electrodynamics and waves in the low-frequency range. With the aid of ground-based optical data, I performed three studies about field-aligned currents (FACs) and Alfvén waves in the auroral region. The first study presents two types of FACs associated with quasi-static multiple arc systems. The comparison between ``unipolar'' and ``multipolar'' FAC systems provides insights in understanding the multiplicity of auroral arcs. The second study presents the statistical relation between Alfvén waves and large-scale FACs. It is found that Alfvénic fluctuations occur over a much wider range of locations and conditions than previously reported. The third study presents the first statistical survey of suprathermal electron bursts (STEBs) in the ionospheric Alfvén resonator. The case event presented in this study demonstrates both normal and inverse dispersion in energy and pitch angle spectrograms of adjacent suprathermal electron bursts. Observations presented in these studies provide important constraints in testing models of electron acceleration and theories of auroral arc generation.en_US
dc.identifier.citationWu, J. (2020). Static and Alfvénic Electrodynamics in the Auroral Region (Doctoral thesis, University of Calgary, Calgary, Canada). Retrieved from https://prism.ucalgary.ca.en_US
dc.identifier.doihttp://dx.doi.org/10.11575/PRISM/38035
dc.identifier.urihttp://hdl.handle.net/1880/112325
dc.publisher.facultyScienceen_US
dc.publisher.institutionUniversity of Calgaryen
dc.rightsUniversity of Calgary graduate students retain copyright ownership and moral rights for their thesis. You may use this material in any way that is permitted by the Copyright Act or through licensing that has been assigned to the document. For uses that are not allowable under copyright legislation or licensing, you are required to seek permission.en_US
dc.subjectspace physicsen_US
dc.subject.classificationPhysicsen_US
dc.titleStatic and Alfvénic Electrodynamics in the Auroral Regionen_US
dc.typedoctoral thesisen_US
thesis.degree.disciplinePhysics & Astronomyen_US
thesis.degree.grantorUniversity of Calgaryen_US
thesis.degree.nameDoctor of Philosophy (PhD)en_US
ucalgary.item.requestcopytrueen_US
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