The study of interplanetary shocks, geomagnetic storms, and substorms with the WINDMI model
| dc.contributor.advisor | Horton, C. W. (Claude Wendell), 1942- | en |
| dc.creator | Mays, Mona Leila | en |
| dc.date.accessioned | 2011-03-24T20:45:57Z | en |
| dc.date.available | 2011-03-24T20:45:57Z | en |
| dc.date.issued | 2009-08 | en |
| dc.description | text | en |
| dc.description.abstract | WINDMI is a low dimensional plasma physics-based model of the coupled magnetosphere-ionosphere system. The nonlinear system of ordinary differential equations describes the energy balance between the basic nightside components of the system using the solar wind driving voltage as input. Of the eight dynamical variables determined by the model, the region 1 field aligned current and ring current energy is compared to the westward auroral electrojet AL index and equatorial geomagnetic disturbance storm time Dst index. The WINDMI model is used to analyze the magnetosphere-ionosphere system during major geomagnetic storms and substorms which are community campaign events. Numerical experiments using the WINDMI model are also used to assess the question of how much interplanetary shock events contribute to the geoeffectiveness of solar wind drivers. For two major geomagnetic storm intervals, it is found that the magnetic field compressional jump is important to producing the changes in the AL index. Further, the WINDMI model is implemented to compute model AL and Dst predictions every ten minutes using real-time solar wind data from the ACE satellite as input. Real-Time WINDMI has been capturing substorm and storm activity, as characterized by the AL and Dst indices, reliably since February 2006 and is validated by comparison with ground-based measurements of the indices. Model results are compared for three different candidate input solar wind driving voltage formulas. Modeling of the Dst index is further developed to include the additional physical processes of tail current increases and sudden commencement. A new model, based on WINDMI, is developed using the dayside magnetopause and magnetosphere current systems to model the magnetopause boundary motion and the dayside region 1 field aligned current which is comparable to the auroral upper AU index. | en |
| dc.description.department | Physics | en |
| dc.format.medium | electronic | en |
| dc.identifier.uri | http://hdl.handle.net/2152/10703 | en |
| dc.language.iso | eng | en |
| dc.rights | Copyright is held by the author. Presentation of this material on the Libraries' web site by University Libraries, The University of Texas at Austin was made possible under a limited license grant from the author who has retained all copyrights in the works. | en |
| dc.subject | WINDMI | en |
| dc.subject | Coupled magnetosphere-ionosphere system | en |
| dc.subject | Field aligned current | en |
| dc.subject | Ring current energy | en |
| dc.subject | Auroral electrojet AL index | en |
| dc.subject | Equatorial geomagnetic disturbance storm time Dst index | en |
| dc.subject | Geomagnetic storms | en |
| dc.subject | Solar wind drivers | en |
| dc.title | The study of interplanetary shocks, geomagnetic storms, and substorms with the WINDMI model | en |
| thesis.degree.department | Physics | en |
| thesis.degree.discipline | Physics | en |
| thesis.degree.grantor | The University of Texas at Austin | en |
| thesis.degree.level | Doctoral | en |
| thesis.degree.name | Doctor of Philosophy | en |