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PREEVENTS Track 2: Collaborative Research: Comprehensive Hazard Analysis for Resilience to Geomagnetic Extreme Disturbances

PREEVENTS Track 2: Collaborative Research: Comprehensive Hazard Analysis for Resilience to Geomagnetic Extreme Disturbances
预防措施轨道 2:协作研究:地磁极端扰动恢复能力的综合危害分析
批准号:
1663770
负责人:
Michael Liemohn
金额:
$118.37万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2017
资助国家:
美国
项目状态:
已结题
起止时间:
2017-09-01 至 2023-08-31

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中文摘要
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英文摘要
Extreme solar storms threaten society, in part, via Geomagnetically Induced Currents (GICs) which damage power transmission systems. A space weather extreme event would devastate the US, costing more than $2T and leaving hundreds of millions without electricity for more than a month. The National Space Weather Action Plan calls for an immediate increase in research and improvements to our predictive capabilities to address this threat. This proposed work will make use of NSF funded data sources (AMPERE, SUPERMAG, and EarthScope) to improve existing models with in the Space Weather Modeling Framework and to generate a new tool for GIC prediction that could easily be transitioned to operations at NOAA's Space Weather Prediction Center.Comprehensive Hazard Analysis for Resilience to Geomagnetic Extreme Disturbances (CHARGED) applies experts in various disciplines to create a fully coupled, physics-based model of GICs that includes the magnetosphere, ionosphere, and solid Earth together with validation against state-of-the art globally distributed observations. The Space Weather Modeling Framework (SWMF) will be improved with realistic particle precipitation and ionospheric conductance physics. A global 3D finite-difference time-domain (FDTD) model will be used to propagate the ionosphere signal through the ground while accounting for the oceans and variable lithosphere conductivity. This model will be validated using the best available in-situ and remote data to determine its predictive accuracy. The relationship between solar driving and GICs will be explored for both historical and idealized extreme events. The project will yield fundamental new understanding of the processes leading to extreme GIC events (solicitation target 1), and expand our capability to model and forecast GIC hazards (target 2). The resulting coupled system could form a natural extension to the operational SWMF version currently at NOAA.
期刊论文(42)
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会议论文
Instigators of future change in magnetospheric physics
磁层物理学未来变革的推动者
DOI: 10.1002/9781119815624.ch47
发表时间: 2021
期刊: Magnetospheres in the Solar System
影响因子: --
作者: [Liemohn, M. W.]
通讯作者: Liemohn, M. W.
DOI: 10.1029/2022sw003102
发表时间: 2022
期刊: Space Weather
影响因子: 3.7
作者: [Liemohn, Michael W., Adam, Joshua G., Ganushkina, Natalia Yu]
通讯作者: Ganushkina, Natalia Yu
Recreating the Horizontal Magnetic Field at Colaba During the Carrington Event With Geospace Simulations
通过地球空间模拟重现卡林顿事件期间科拉巴的水平磁场
DOI: 10.1029/2020sw002585
发表时间: 2021
期刊: Space Weather
影响因子: 3.7
作者: [Blake, Seán P., Pulkkinen, Antti, Schuck, Peter W., Glocer, Alex, Oliveira, Denny M., Welling, Daniel T., Weigel, Robert S., Quaresima, Gary]
通讯作者: Quaresima, Gary
Communicating Uncertainty and Reliability in Space Weather Data, Models, and Applications
传达空间天气数据、模型和应用中的不确定性和可靠性
DOI: 10.1029/2018sw002083
发表时间: 2018
期刊: Space Weather
影响因子: 3.7
作者: [Knipp, Delores J., Hapgood, Michael A., Welling, Daniel]
通讯作者: Welling, Daniel
35
    Synoptic Investigation of Extreme Events: Sun to the Upper Atmosphere
    Collaborative Research: GEM: Investigation of UT Dependence of Magnetic Storm Strength
    Collaborative Research: Global Response of the Martian Thermosphere to Energetic Pickup Ions
    GEM: Assessing the Storm-Time Magnetic Distortion in the Inner Magnetosphere
    海外基金