Overview of Jovian Aurora's observed features and its possible origin

dc.contributor.advisorHill, Thomas W.en_US
dc.creatorGong, Binen_US
dc.date.accessioned2009-06-04T06:56:20Zen_US
dc.date.available2009-06-04T06:56:20Zen_US
dc.date.issued2003en_US
dc.description.abstractAs on Earth, Jupiter's auroral emission comes from the upward Birkeland currents. The VIP4 magnetic field model maps the main oval to the middle magnetosphere (r ∼ 30 RJ). However, the interpretation of the observed features of the jovian aurora and its link to the middle magnetosphere remains an open question. This thesis reviews the main observational features and existing models of Jupiter's aurora. After comparing the merits and disadvantages of each model, we outline future possible improvements of the models.en_US
dc.format.extent31 p.en_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.callnoTHESIS PHYS. 2003 GONGen_US
dc.identifier.citationGong, Bin. "Overview of Jovian Aurora's observed features and its possible origin." (2003) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/17593">https://hdl.handle.net/1911/17593</a>.en_US
dc.identifier.urihttps://hdl.handle.net/1911/17593en_US
dc.language.isoengen_US
dc.rightsCopyright is held by the author, unless otherwise indicated. Permission to reuse, publish, or reproduce the work beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.subjectAstronomyen_US
dc.subjectAstrophysicsen_US
dc.titleOverview of Jovian Aurora's observed features and its possible originen_US
dc.typeThesisen_US
dc.type.materialTexten_US
thesis.degree.departmentPhysicsen_US
thesis.degree.disciplineNatural Sciencesen_US
thesis.degree.grantorRice Universityen_US
thesis.degree.levelMastersen_US
thesis.degree.nameMaster of Scienceen_US
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