郭金涵，5168cc银河免费下载安装博士后。2024年于南京大学大学5168cc银河免费下载安装获得天文学博士学位，期间在比利时鲁汶大学数学系联合培养。现已作为第一作者/通讯作者发表SCI论文10篇，引用200余次。曾获“博士后创新人才支持计划”资助、国际天文联合会（IAU）优秀博士论文提名奖、亚太物理学会-等离子体物理分会U30青年科学家奖、亚太太阳物理会议最佳论文奖等。
研究生课程《太阳活动区物理》：太阳磁场的观测、建模与理论描述
日冕与行星际物理，磁流体力学数值模拟，包括：
（1）基于观测数据限制/驱动的太阳爆发和行星际介质动力学的数值建模；
（2）暗条的形成、动力学和精细结构；
（3）日冕三维磁场的数值重构方法；
（4）太阳爆发相关的波动现象;
（太阳活动区的三维磁场演化：Guo et al. 2024, ApJ）
（暗条物质形成与振荡：Guo et al. 2021, ApJ）
（日冕磁绳模型：Schmieder, Guo & Poedts, 2024, RMPP）
（日冕极紫外波：Y. W. Li, Guo et al. 2025, A&A）
发表论文详见：https://www.researchgate.net/profile/Jinhan-Guo?ev=hdr_xprf
[1] J. H. Guo, Y. W. Ni, Y. Qiu, Z. Zhong, Y. Guo, P. F. Chen, Magnetic Twists of Solar Filaments, The Astrophysical Journal, 917, 81 (2021).
[2] J. H. Guo, Y. H. Zhou, Y. Guo, Y. W. Ni, J. T. Karpen, P. F. Chen, Formation and Characteristics of Filament Threads in Double-Dipped Magnetic Flux Tubes, The Astrophysical Journal, 920, 131 (2021).
[3] J. H. Guo, Y. W. Ni, Y. H. Zhou, Y. Guo, B. Schmieder, P. F. Chen, Prominence fine structures in weakly twisted and highly twisted magnetic flux ropes, Astronomy & Astrophysics, 667, A89 (2022).
[4] J. H. Guo, Y. W. Ni, Z. Zhong, Y. Guo, C. Xia, H. T. Li, S. Poedts, B. Schmieder, P. F. Chen, B. Schmieder, 2023, Thermodynamic and Magnetic Topology Evolution of the X1.0 Flare on 2021 October 28 Simulated by a Data-driven Radiative Magnetohydrodynamic Model, The Astrophysical Journal Supplement Series, 266:3, 20pp (2023).
[5] J. H. Guo, Y. Qiu, Y.W. Ni, Y. Guo, C. Li, Y.H. Gao, B. Schmieder, S. Poedts, P.F. Chen, 2023, Understand- ing the Lateral Drifting of an Erupting Filament with a Data-constrained Magnetohydrodynamic Simulation, The Astrophysical Journal, 956, 119, 16pp (2023).
[6] J. H. Guo, Y. W. Ni, Y. Guo, C. Xia, B. Schmieder, S. Poedts, Z. Zhong, Y. H. Zhou, F. Yu, P. F. Chen, Data-driven modeling of coronal magnetic flux rope: from birth to death, 2023, The Astrophysical Journal, 961:140, 17pp (2024).
[7] J. H. Guo, L. Linan, S. Poedts, Y. Guo, A. Lani, B. Schmieder, M. Brchnelova, B. Perri, T. Baratashvili, Y. W. Ni, P. F. Chen, Modelling the propagation of coronal mass ejections with COCONUT: implementation of the Regularized Biot-Savart Laws flux rope model, Astronomy & Astrophysics, 683, A54 (2024).
[8] J. H. Guo, L. Linan, S. Poedts, Y. Guo, B. Schmieder, A. Lani, Y. W. Ni, M. Brchnelova, B. Perri, T. Baratashvili, Y. W. Ni, S. T. Li, P. F. Chen, Dependence of coronal mass ejections on the morphology and toroidal flux of their source magnetic flux ropes, Astronomy & Astrophysics, 683, A54 (2024).
[9] J. H. Guo, Y. W. Ni, B. Schmieder, Y. Guo, C. Xia et al., The Birth of a Major Coronal Mass Ejection with Intricate Magnetic Structure from Multiple Active Regions, The Astrophysical Journal, 983, 48 (2025).
[10] Haopeng Wang, Jinhan Guo, Liping Yang, Stefaan Poedts, Fan Zhang, Andrea Lani, Tinatin Baratashvili, Luis Linan, Rong Lin, Yang Guo, SIP-IFVM: An efficient time-accurate implicit MHD model of corona and CME with strong magnetic field, Astronomy & Astrophysics, 693, A257 (2025).