太阳风时间变化的 Helio1D 建模:Multi-VP 和 1D MHD 之间的接口,用于未来 L1 的业务预报

IF 3.4 2区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Journal of Space Weather and Space Climate Pub Date : 2024-05-23 DOI:10.1051/swsc/2024018
R. Kieokaew, Rui Pinto, Evangelia Samara, C. Tao, M. Indurain, Benoit Lavraud, Antoine Brunet, V. Génot, Alexis Rouillard, Nicolas André, Sébastien Bourdarie, Christos Katsavrias, Fabien Darrouzet, Benjamin Grison, Ioannis Daglis
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引用次数: 0

摘要

为地球上游的太阳风状况预测开发一个自动管道,是从空间气象研究过渡到运行的重要一步。我们开发了一个名为 "Helio1D "的原型管道,用于模拟环境太阳风状况,包括 L1 的风速、密度、温度和切向磁场的时间剖面,可提前 4 天进行模拟。原型管道将提供 0.14 AU 太阳风每日预测的 MULTI-VP 日冕模型和将太阳风传播到 1 AU 的一维磁流体动力学(MHD)模型连接起来。作为未来开发性能更好的运行管道的一部分,我们目前的工作重点是Helio1D的概念验证、初步实施和验证。在此,我们首先使用威尔科克斯空间天文台提供的同步磁图作为MULTI-VP日冕部分的输入,对2004-2013年和2017-2018年期间的Helio1D进行基准测试。使用经典的点对点指标,我们发现Helio1D在所有时间间隔内的表现都不如27天重现模型,而在太阳周期晚期的下降阶段则优于4天持续模型。作为补充分析,我们利用快速动态时间扭曲技术评估了Helio1D与观测数据之间的时间和幅度差异,从而讨论了Helio1D的注意事项,并解决了校准问题,以提高Helio1D的性能。此外,我们还并行模拟了几种太阳风条件,总共 21 个剖面与各种虚拟目标相对应,以提供不确定性。虽然我们的原型管道显示出的结果不如现有工作那么令人满意,但它是完全自动化的,计算速度也很快,这两点都是业务预报所需要的。我们还讨论了未来的改进策略,以实现性能更佳的管道。
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Helio1D modeling of temporal variation of solar wind: interfacing between Multi-VP and 1D MHD for future operational forecasting at L1
Developing an automated pipeline for solar-wind condition prediction upstream of Earth is an important step for transitioning from space weather research to operation. We develop a prototype pipeline called “Helio1D” to model ambient solar wind conditions comprising temporal profiles of wind speed, density, temperature and tangential magnetic field at L1 up to 4 days in advance. The prototype pipeline connects MULTI-VP coronal model that provides daily predictions of the solar wind at 0.14 AU and a 1D magnetohydrodynamics (MHD) model that propagates the solar wind to 1 AU. As a part of development towards a better performing operational pipeline in the future, our present work focuses on the proof-of-concept, initial implementation, and validation of Helio1D. Here, we first benchmark Helio1D using the synoptic magnetograms provided by Wilcox Space Observatory as inputs to the coronal part of MULTI-VP for the intervals in 2004 -- 2013 and 2017 -- 2018. Using the classic point-to-point metrics, it is found that Helio1D underperforms the 27-day recurrence model for all time intervals, while outperforms the 4-day persistence model in the late declining phase of the solar cycle. As a complementary analysis, we evaluate the time and magnitude differences between Helio1D and the observations by exploiting the Fast Dynamic Time Warping technique, which allows us to discuss Helio1D caveats and address calibration to improve the Helio1D performance. Furthermore, we model several solar wind conditions in parallel, for a total of 21 profiles corresponding to various virtual targets to provide uncertainties. Although our prototype pipeline shows less satisfactory results compared to existing works, it is fully automated and computationally fast, both of which are desirable qualities for operational forecasting. Our strategies for future improvements towards a better performing pipeline are addressed.
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来源期刊
Journal of Space Weather and Space Climate
Journal of Space Weather and Space Climate ASTRONOMY & ASTROPHYSICS-GEOCHEMISTRY & GEOPHYSICS
CiteScore
6.90
自引率
6.10%
发文量
40
审稿时长
8 weeks
期刊介绍: The Journal of Space Weather and Space Climate (SWSC) is an international multi-disciplinary and interdisciplinary peer-reviewed open access journal which publishes papers on all aspects of space weather and space climate from a broad range of scientific and technical fields including solar physics, space plasma physics, aeronomy, planetology, radio science, geophysics, biology, medicine, astronautics, aeronautics, electrical engineering, meteorology, climatology, mathematics, economy, informatics.
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