Mapping magnetic flux tubes and field aligned currents using two representative magnetospheric models
dc.contributor.advisor | Hill, Thomas W. | en_US |
dc.creator | Ding, Cheng | en_US |
dc.date.accessioned | 2009-06-04T00:45:00Z | en_US |
dc.date.available | 2009-06-04T00:45:00Z | en_US |
dc.date.issued | 1993 | en_US |
dc.description.abstract | Among available quantitative magnetospheric models, the Tsyganenko models represent empirical modeling, while the Toffoletto and Hill model is theoretical analysis. By mapping flux tubes between the ionosphere and the magnetosphere, those two models are analyzed and compared. Both the implied and actual field-aligned currents (FAC) are calculated in both models. The implied FAC, required to maintain the model field in magnetostatic equilibrium and given by the Vasyliunas equation, has the same order of magnitude as observational data, even in non-equilibrium models. The actual FAC, given by Ampere's law, is much smaller than the implied FAC, which means no large extraneous FAC is included in those models. Several new approaches imply that none of these models are in magnetostatic equilibrium, while the discrepancies are considerably larger for the Tsyganenko models. The magnetic effects of a preliminary FAC model have been evaluated in the Toffoletto and Hill theoretical model. | en_US |
dc.format.extent | 75 p. | en_US |
dc.format.mimetype | application/pdf | en_US |
dc.identifier.callno | THESIS SP. SCI. 1993 DING | en_US |
dc.identifier.citation | Ding, Cheng. "Mapping magnetic flux tubes and field aligned currents using two representative magnetospheric models." (1993) Master’s Thesis, Rice University. <a href="https://hdl.handle.net/1911/13714">https://hdl.handle.net/1911/13714</a>. | en_US |
dc.identifier.uri | https://hdl.handle.net/1911/13714 | en_US |
dc.language.iso | eng | en_US |
dc.rights | Copyright 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.subject | Geophysics | en_US |
dc.subject | Astronomy | en_US |
dc.subject | Astrophysics | en_US |
dc.subject | Plasma physics | en_US |
dc.title | Mapping magnetic flux tubes and field aligned currents using two representative magnetospheric models | en_US |
dc.type | Thesis | en_US |
dc.type.material | Text | en_US |
thesis.degree.department | Space Science | en_US |
thesis.degree.discipline | Natural Sciences | en_US |
thesis.degree.grantor | Rice University | en_US |
thesis.degree.level | Masters | en_US |
thesis.degree.name | Master of Science | en_US |
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