Geomagnetically induced currents (gics), which are strongly related to the change rate of geomagnetic field, pose a large hazard to the important infrastructures, such as powerlines and pipelines,…

This is a $652,409 grant award from the NASA Shared Services Center to the University of Texas at Arlington (UTA) for a research project on geomagnetically induced currents (GICs) and their impact on critical infrastructure. The goal is to examine the various forcing terms driving multi-scale variations in geomagnetic disturbances through magnetosphere-ionosphere coupled simulations. This supports advances in numerical models for resolving these complex, multi-scale geomagnetic disturbances. The award is not set aside and represents UTA's extensive research and development capabilities, particularly in areas like aerospace engineering, materials science, and space physics. UTA is a Hispanic-Serving and Minority Institution within the University of Texas System, which has a significant portfolio of federal research contracts and grants across scientific disciplines.

Geomagnetically induced currents (gics), which are strongly related to the change rate of geomagnetic field, pose a large hazard to the important infrastructures, such as powerlines and pipelines, especially during geomagnetic super storms. IT is essential to understand the magnetospheric and ionospheric processes responsible for the geomagnetic disturbances (GMD) during space weather events in order to improve the preparedness of society to the space weather impact. Recently significant progresses have been made in both observations and simulations to improve the description and understanding of gics. A wide range of spacecraft and ground datasets has been utilized to analyze gics and their correlation with drivers. Meanwhile, both first-principles physical models (MHD model coupled with ionosopheric electrodynamic model) and empirical models have been applied to the calculation of the geomagnetic perturbations. The ground conductivity model, which plays a crucial role to estimate the geoelectric field from geomagnetic disturbance (GMD), has been improved from 1-d to 3-d. However, a comprehensive understanding of the impact of different processes on the multi-scale geomagnetic disturbances is lacking, yet IT remains fundamental to correctly interpret and specify gics. Further, IT is clear that small spatial scale magnetic perturbations with large amplitudes are a contributor to the GIC problem, but the underlying physics of these localized effects remains unclear [ngwira and pulkkinen, 2019]. The goal of this project is to examine the relative significance of different forcing terms in driving the multi-scale variations of geomagnetic disturbances through magnetosphere-ionosphere coupled simulations. Specifically, we will address the following three science questions (SQ): (1) what is the role of the ionospheric and thermospheric processes in producing GEO- magnetic disturbances on the ground? Proposed study: use MHD-GCM numerical models with expanded coupling that includes thermospheric processes such as the neutral dynamo to examine disturbance generation and to compare with observations. (2) how does the combined m-i system produce geomagnetic disturbances of different spatial and temporal scales? Proposed study: with high resolution MHD-GCM coupled model, explore processes leading to different scales of disturbances, including solar wind conditions, conductance and neutral-wind perturbations driven by atmospheric waves. (3) how do magnetic perturbations manifest as geoelectric fields, and how much does the earth conductivity model affect this conversion? Proposed study: examine the frequency dependence of geoelectric field conversion, decompose the geoelectric field by its contributions from different geospace regions, and convolve numerical results with 1D and 3D models of earth s conductivity. This investigation will make significant contributions to the scientific objectives of the NASA LWS focus science topic 3: magnetospheric and ionospheric processes responsible for rapid geomagnetic changes. Specifically, IT will improve modeling of geomagnetic disturbances and geoelectric field during disturbed periods and to improve understanding of the role of solar wind, magnetosphere, ionosphere and thermosphere in driving geomagnetic variation and geoelectric field. Furthermore, this investigation will make important contributions to science questions from the heliophysics roadmap and decadal survey. We would intend to interact with space physicists in the team to work on problems of overlapping interest that may be identified.