课题基金 / 基金详情

SWQU: NextGen Space Weather Modeling Framework Using Data, Physics and Uncertainty Quantification

SWQU: NextGen Space Weather Modeling Framework Using Data, Physics and Uncertainty Quantification
SWQU:使用数据、物理和不确定性量化的下一代空间天气建模框架
批准号:
2027555
负责人:
Gabor Toth
金额:
$286.0万
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2020
资助国家:
美国
项目状态:
已结题
起止时间:
2020-09-01 至 2024-08-31

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中文摘要
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英文摘要
This project will initiate development of the NextGen Space Weather Modeling Framework (NextGen SWMF) by bringing together experts in space and plasma physics, data assimilation, uncertainty quantification and cyberinfrastructure. Space weather results from solar activity that can impact the space environment of the Earth and damage our technological systems as well as expose pilots and astronauts to harmful radiation. Extreme events could knock out the power grid with a recovery time of months and cause about $2 trillion damage. Much of the impacts can be avoided or mitigated by timely and reliable space weather forecast. The NextGen Space Weather Modeling Framework will employ computational models from the surface of the Sun to the surface of Earth in combination with assimilation of observational data to provide optimal probabilistic space weather forecasting. The model will run efficiently on the next generation of supercomputers to predict space weather about one day or more before the impact occurs. The project will concentrate on forecasting major space weather events generated by coronal mass ejections.Current space weather prediction employs first-principles and/or empirical models. While these provide useful information, their accuracy, reliability and forecast window need major improvements. Data assimilation has the potential to significantly improve model performance, as has been successfully done in terrestrial weather forecast. However, to allow for the sparsity of satellite observations, different data assimilation methods have to be employed. NextGen SWMF model will start from the Sun with an ensemble of simulations that span the uncertain observational and model parameters. Using real time and past observations, the model will strategically down-select to a high performing subset. Next, the down-selected ensemble will be extended by varying uncertain parameters and the simulation continued to the next data assimilation point. The final ensemble will provide a probabilistic forecast of the space weather impacts. Finding the optimal algorithm that produces the best prediction with minimal uncertainty is a complex and very challenging task that requires developing, implementing and perfecting novel data assimilation and uncertainty quantification methods. To make these ensemble simulations run faster than real time, the most expensive parts of the model need to run efficiently on the current and future supercomputers, which employ graphical processing units (GPUs) in addition to the traditional multi-core CPUs. The main product of this project will be the Michigan Sun-To-Earth Model with Quantified Uncertainty and Data Assimilation (MSTEM-QUDA).This award is made as a part of the joint NSF-NASA pilot program on Next Generation Software for Data-driven Models of Space Weather with Quantified Uncertainties (SWQU). It is supported by NSF Divisions of Astronomical Sciences, Atmospheric and Geospace Sciences, Mathematical Sciences, and Physics. All software developed as a result of this award will be made available by the awardee free of charge for non-commercial use; the software license will permit modification and redistribution of the software free of charge for non-commercial use.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.
期刊论文(12)
专著(0)
科研奖励(0)
会议论文
Three‐Dimensional Structure of the Corona During WHPI Campaign Rotations CR‐2219 and CR‐2223
WHPI 活动轮换 CR-2219 和 CR-2223 期间日冕的三维结构
DOI: 10.1029/2022ja030406
发表时间: 2022
期刊: Journal of Geophysical Research: Space Physics
影响因子: --
作者: [Lloveras, D. G., Vásquez, A. M., Nuevo, F. A., Frazin, R. A., Manchester, W., Sachdeva, N., Van der Holst, B., Lamy, P., Gilardy, H.]
通讯作者: Gilardy, H.
DOI: 10.1029/2021sw002928
发表时间: 2022-07
期刊: Space Weather
影响因子: --
作者: [Daniel Iong;Yang Chen;G. Tóth;S. Zou;Tuija Pulkkinen;Jiaen Ren;E. Camporeale;T. Gombosi]
通讯作者: Daniel Iong;Yang Chen;G. Tóth;S. Zou;Tuija Pulkkinen;Jiaen Ren;E. Camporeale;T. Gombosi
Simulating Solar Maximum Conditions Using the Alfvén Wave Solar Atmosphere Model (AWSoM)
使用阿尔文波太阳大气模型 (AWSoM) 模拟太阳极大值条件
DOI: 10.3847/1538-4357/ac307c
发表时间: 2021
期刊: The Astrophysical Journal
影响因子: --
作者: [Sachdeva, Nishtha, Tóth, Gábor, Manchester, Ward B., van der Holst, Bart, Huang, Zhenguang, Sokolov, Igor V., Zhao, Lulu, Shidi, Qusai Al, Chen, Yuxi, Gombosi, Tamas I.]
通讯作者: Gombosi, Tamas I.
Tomography of the Solar Corona with the Metis Coronagraph I: Predictive Simulations with Visible-Light Images
使用 Metis Coronagraph I 进行日冕层析成像:使用可见光图像进行预测模拟
DOI: 10.1007/s11207-022-02047-9
发表时间: 2022
期刊: Solar Physics
影响因子: 2.8
作者: [Vásquez, Alberto M., Nuevo, Federico A., Frassati, Federica, Bemporad, Alessandro, Frazin, Richard A., Romoli, Marco, Sachdeva, Nishtha, Manchester, Ward B.]
通讯作者: Manchester, Ward B.
9
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