2021年10月28日X1.0级耀斑的热动力学及磁拓扑演化的数据驱动模拟研究（英文）

【作者】 郭金涵； 倪仪伟； 郭洋； 钟泽； 陈鹏飞； 夏莼；

【机构】 School of Astronomy and Space Science, Nanjing University； Institute of Frontier and Interdisciplinary Science, Shandong University； School of Physics and Astronomy, Yunnan University；

【摘要】 <正>Filament eruptions, flares and coronal mass ejections (CMEs) are the energetic manifestations of the solar magnetic field, which are related to abundant astrophysical processes, such as magnetic reconnection, heating, waves and so on. We attempt to reproduce typical observational features of the X1.0 class flare at the start of the solar cycle 25 with a data-driven simulation. And we analyze the thermodynamic and magnetic topology evolution during the eruption.更多还原