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

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    Author
    Gong, Bin
    Date
    2003
    Advisor
    Hill, Thomas W.
    Degree
    Master of Science
    Abstract
    As 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.
    Keyword
    Astronomy; Astrophysics
    Citation
    Gong, Bin. "Overview of Jovian Aurora's observed features and its possible origin." (2003) Master’s Thesis, Rice University. https://hdl.handle.net/1911/17593.
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    Managed by the Digital Scholarship Services at Fondren Library, Rice University
    Physical Address: 6100 Main Street, Houston, Texas 77005
    Mailing Address: MS-44, P.O.BOX 1892, Houston, Texas 77251-1892
    Site Map