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EUropean Heliospheric FORecasting Information Asset 2.0

机译:欧洲光星预测信息资产2.0

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Aims : This paper presents a H2020 project aimed at developing an advanced space weather forecasting tool, combining the MagnetoHydroDynamic (MHD) solar wind and coronal mass ejection (CME) evolution modelling with solar energetic particle (SEP) transport and acceleration model(s). The EUHFORIA 2.0 project will address the geoeffectiveness of impacts and mitigation to avoid (part of the) damage, including that of extreme events, related to solar eruptions, solar wind streams, and SEPs, with particular emphasis on its application to forecast geomagnetically induced currents (GICs) and radiation on geospace. Methods : We will apply innovative methods and state-of-the-art numerical techniques to extend the recent heliospheric solar wind and CME propagation model EUHFORIA with two integrated key facilities that are crucial for improving its predictive power and reliability, namely (1) data-driven flux-rope CME models, and (2) physics-based, self-consistent SEP models for the acceleration and transport of particles along and across the magnetic field lines. This involves the novel coupling of advanced space weather models. In addition, after validating the upgraded EUHFORIA/SEP model, it will be coupled to existing models for GICs and atmospheric radiation transport models. This will result in a reliable prediction tool for radiation hazards from SEP events, affecting astronauts, passengers and crew in high-flying aircraft, and the impact of space weather events on power grid infrastructure, telecommunication, and navigation satellites. Finally, this innovative tool will be integrated into both the Virtual Space Weather Modeling Centre (VSWMC, ESA) and the space weather forecasting procedures at the ESA SSCC in Ukkel (Belgium), so that it will be available to the space weather community and effectively used for improved predictions and forecasts of the evolution of CME magnetic structures and their impact on Earth. Results : The results of the first six months of the EU H2020 project are presented here. These concern alternative coronal models, the application of adaptive mesh refinement techniques in the heliospheric part of EUHFORIA, alternative flux-rope CME models, evaluation of data-assimilation based on Karman filtering for the solar wind modelling, and a feasibility study of the integration of SEP models.
机译:目的:本文介绍了一个H2020项目,旨在开发先进的空间天气预报工具,将磁力动力学(MHD)太阳能和冠状大规模喷射(CME)进化建模与太阳能粒子(SEP)运输和加速模型相结合。 Euhforia 2.0项目将解决影响和缓解的地理信息源,以避免(部分)损坏,包括与太阳爆发,太阳风流和SEP有关的极端事件,特别强调其预测地磁诱导的电流的应用(GICS)和地球空间的辐射。方法:我们将采用创新方法和最先进的数值技术,以扩展最近的恒星太阳能和CME传播模型Euhforia,这是两个集成的关键设施,这对于提高其预测功率和可靠性至关重要,即(1)数据 - 驱动的磁通绳CME模型,(2)基于物理的,自我一致的SEP模型,用于沿下和穿过磁场线的加速和运输粒子。这涉及高级空间天气模型的新耦合。此外,在验证升级的EUHForia / SEP模型后,它将耦合到现有的GIC和大气辐射传输模型。这将导致来自SEP事件的辐射危害的可靠预测工具,影响高飞机的宇航员,乘客和船员,以及空间天气事件对电网基础设施,电信和导航卫星的影响。最后,这种创新工具将集成到虚拟空间天气建模中心(VSWMC,ESA)和Ukkel(比利时)的ESA SSCC中的空间天气预报程序,以便它将可供空天天气社区和有效地使用用于改进CME磁性结构的进化的预测和预测及其对地球的影响。结果:此处提出了欧盟H2020项目的前六个月的结果。这些涉及的替代冠状模型,在Euhforia的恒星部分中的应用,替代助焊绳CME模型中的应用,基于Karman滤波的数据同化评估,对太阳风模拟的可行性研究SEP型号。

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