Hemispheric Asymmetries of Magnetosphere-Ionosphere-Thermosphere Dynamics

[摘要] The geospace environment, comprised of the magnetosphere-ionosphere-thermosphere system, is a highly variable and non-linearly coupled region. The dynamics of the system are driven primarily by electromagnetic and particle radiation emanating from the Sun that occasionally intensify into what are known as solar storms. Understanding the interaction of these storms with the near Earth space environment is essential for predicting and mitigating the risks associated with space weather that can irreparably damage spacecraft, harm astronauts, disrupt radio and GPS communications, and even cause widespread power outages.The geo-effectiveness of solar storms has hemispheric, seasonal, local time, universal time, and latitudinal dependencies. This dissertation investigates those dependencies through a series of four concentrated modeling efforts. The first study focuses on how variations in the solar wind electric field impact the thermosphere at different times of the day. Idealized simulations using the Global Ionosphere Thermosphere Model (GITM) revealed that perturbations in thermospheric temperature and density were greater when the universal time of storm onset was such that the geomagnetic pole was pointed more towards the sun. This universal time effect was greater in the southern hemisphere where the offset of the geomagnetic pole is larger. The second study presents a model validation effort using GITM and the Thermosphere Ionosphere Electrodynamics General Circulation Model (TIE-GCM) compared to GPS Total Electron Content (TEC) observations. The results were divided into seasonal, regional, and local time bins finding that the models performed best near the poles and on the dayside. Diffuse aurora created by electron loss in the inner magnetosphere is an important input to GITM that has primarily been modeled using empirical relationships. In the third study, this was addressed by developing the Hot Election Ion Drift Integrator (HEIDI) ring current model to include a self-consistent description of the aurora and electric field. The model was then coupled to GITM, allowing for a more physical aurora. Using this new configuration in the fourth study, the ill-constrained electron scattering rate was shown to have a large impact on auroral results. This model was applied to simulate a geomagnetic storm during each solstice. The hemispheric asymmetry and seasonal dependence of the storm-time TEC was investigated, finding that northern hemisphere winter storms are most geo-effective when the North American sector is on the dayside.Overall, the research presented in this thesis strives to accomplish two major goals. First, it describes an advancement of a numerical model of the ring current that can be further developed and used to improve our understanding of the interactions between the ionosphere and magnetosphere. Second, the time and spatial dependencies of the geospace response to solar forcing were discovered through a series of modeling efforts. Despite these advancements, there are still numerous open questions, which are also discussed.

[发布机构] University of Michigan

[效力级别] Atmospheric

[关键词] Hemispheric Asymmetries Magnetosphere Ionosphere Thermosphere;Atmospheric;Oceanic and Space Sciences;Science;Atmospheric, Oceanic & Space Science