Model generated open-closed field topology maps produced by ISSI team "Magnetic Open Flux And Solar Wind Structuring Of Interplanetary Space"

Open and closed magnetic field topologies of the solar corona generated using four PFSS based coronal models (EUHFORIA, WSA, MULTI-VP, PSI-PFSS) and one full MHD coronal model (PSSI-MHD) using two different types of HMI-ADAPT magnetic field maps (with and without Active Regions (AR) added retrospectively). The magnetograms used are accessible here https://doi.org/10.5281/zenodo.10211762 (Henney, Carl. ‘ADAPT Global Solar Magnetic Maps - 2010 Sep 18-20 (w/ & W/o Farside Active Region Input)’. Zenodo, 28 November 2023). These model outputs were generated by the ISSI team "Magnetic Open Flux And Solar Wind Structuring Of Interplanetary Space" and were used for the paper accessible on Arxiv via this link: https://arxiv.org/abs/2311.04024本数据集涵盖基于势场源面模型（Potential Field Source Surface, PFSS）的四类日冕模型（EUHFORIA、WSA、MULTI-VP、PSI-PFSS）与一款完整磁流体动力学（Magnetohydrodynamics, MHD）日冕模型PSSI-MHD所生成的太阳日冕开放与闭合磁场拓扑结构，其生成过程采用了两类不同的HMI-ADAPT磁场图：分别为回溯性添加活动区（Active Regions, AR）的版本与未添加活动区的版本。所用磁图可通过以下链接获取：https://doi.org/10.5281/zenodo.10211762（Henney, Carl. 《ADAPT全球太阳磁图——2010年9月18-20日（含与不含远端活动区输入数据）》. Zenodo, 2023年11月28日）。 该模型输出结果由国际空间科学研究所（International Space Science Institute, ISSI）下属团队“行星际空间的磁开放通量与太阳风结构（Magnetic Open Flux And Solar Wind Structuring Of Interplanetary Space）”生成，并被用于发表于arXiv的学术论文，论文链接为：https://arxiv.org/abs/2311.04024。