个人简历

2006年毕业于北京师范大学天文系，2006年9月至2011年7月在中国科学院大学攻读空间物理学博士学位，从事日冕太阳风数值模拟研究，获中国科学院优秀博士论文奖。随后在中国科学院国家空间科学中心从事太阳爆发数值模拟研究工作，于2014年12月被聘为副研究员。2013年11月至2015年10月在美国阿拉巴马大学亨茨维尔分校从事博士后研究。
2017年3月到哈尔滨工业大学（深圳）空间科学与应用技术研究院任副教授，2017年12月入选哈尔滨工业大学青年拔尖教授。2018年获国家优秀青年基金。
学术成果：开发了高性能的自适应时空守恒数值磁流体格式和一整套日冕三维磁场重构的新方法；发展了由观测数据直接驱动的太阳活动区磁流体连续演变的数值模式；首次模拟再现日冕磁结构从初现、成形直到爆发的完整动力学过程，开辟了分析爆发的触发机制和初始过程的新途径。在《Nature Communications》、《Astrophysical Journal》等权威期刊发表论文40余篇，被国际同行评价为“引领了一个新的研究热点”。2015年度获美国地球物理学会Basu Early Career Award。主持过多项国家自然科学基金，并作为核心成员参与了多项国家自然科学基金重大项目和重点项目。
教育经历
1 2002-2006 本科，天文学，北京师范大学
2 2006-2011 博士研究生，空间物理学，中国科学院大学
研究与工作经历
1 2011-2013 博士后，空间物理学，中国科学院国家空间科学中心
2 2013-2015 博士后，Space Physics， University of Alabama in Huntsville
3 2015-2016 副研究员，中国科学院国家空间科学中心
4 2017-2018 副教授，哈尔滨工业大学（深圳）
5 2018-至今 教授，哈尔滨工业大学（深圳）
科研项目
2020-2022 深圳市科创委基础研究面上项目，《太阳风暴数值预报研究》
2019-2021 国家自然科学基金优秀青年基金，《太阳爆发数值模式》
2016-2019 国家自然科学基金面上项目，《太阳爆发过程中日冕磁场的重建与分析》
2013-2015 国家自然科学基金青年基金，《太阳爆发活动源区三维非势磁场重构的 MHD 方法研究》
科研成果及奖励
2015 美国地球物理学会（American Geophysical Union) 青年科学家BASU奖
任教和任导师经历
1. 本科生课程《大学物理实验IA，IB》
2. 研究生课程《太阳活动物理》，《等离子体数值模拟方法》
1. 博士研究生：边新凯
2. 硕士研究生：刘志鹏，孙婷婷

研究领域

太阳爆发活动的数据驱动模拟、太阳风暴数值模式、日冕磁场的数值重构方法、高性能磁流体数值计算格式研究。""

近期论文

2019年

1. Zou, P., Jiang, C.W.(#), Feng, X. S., et al. A Two-step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region AR12673, The Astrophysical Journal, 870:97 (2019).
2. Jiang, C. W., Duan A, Feng X, Zou P, Zuo P and Wang Y (2019) Reconstruction of a Highly Twisted Magnetic Flux Rope for an Inter-active-region X-Class Solar Flare. Front. Astron. Space Sci. 6:63. doi: 10.3389/fspas.2019.0006
3. Peng Zou, Chao-Wei Jiang, Feng-Si Wei, and Wen-Da Cao (2019) Can injection model replenish the filaments in weak magnetic environment? Research in Astron. Astrophys, 19, 84-95
4. Peng Zou , Chaowei Jiang* , Fengsi Wei, Pingbing Zuo , and Yi Wang (2019) A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejetion, The Astrophysical Journal, 884, 157-171
5. Aiying Duan, Chaowei Jiang*, Wen He, Xueshang Feng, Peng Zou, and Jun Cui, A Study of Pre-flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes，The Astrophysical Journal, 884:73
2018年
1. Jiang, C. W., Zou, P., Feng, X. S., Hu, Q., Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology, The Astrophysical Journal, 869:13 (2018).
2. Jiang, C. W., Zou, P., Feng, X. S., Hu, Q., Formation and Eruption of an Active Region Sigmoid. II. Magnetohydrodynamic Simulation of a Multistage Eruption, The Astrophysical Journal, 866:96 (2018).
2017年
1. Jiang, C. W., Feng, X.S., Wu, S. T., & Hu, Q., A magnetic bald-patch flare in solar active region 11117, Research in Astronomy and Astrophysics, 17, 93 (2017)
2. Chaowei Jiang, Xiaoli Yan, Xueshang Feng, Aiying Duan, Qiang Hu, Pingbing Zuo, and Yi Wang, Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with a Homologous X-shaped Flare, The Astrophysical Journal, 850, 8 (2017)
3. Yan, X. L., Jiang, C. W., Xue, Z. K., Wang, J. C., Priest, E. R., Yang, L. H., Kong, D. F., Cao, W. D. and Ji, H. S., The Eruption of a Small-scale Emerging Flux Rope as the Driver of an M-class Flare and of a Coronal Mass Ejection, The Astrophysical Journal, 845, 18 (2017)
4. Duan, A. Y., Jiang, C. W., Hu, Q., Zhang, H., Gary, G.A., Wu, S. T., and Cao, J. B., Comparison of Two Coronal Magnetic Field Models to Reconstruct a Sigmoidal Solar Active Region with Coronal Loops, The Astrophysical Journal, 842, 119 (2017)
5. Yun Yang, Xue-Shang Feng, Chao-Wei Jiang, A high-order CESE scheme with a new divergence-free method for MHD numerical simulation, Journal of Computational Physics, 349, 561, (2017)
6. Wensi Wang, Rui Liu, Yuming Wang, Qiang Hu, Chenglong Shen, Chaowei Jiang, Chunming Zhu, Buildup of a highly twisted magnetic flux rope during a solar eruption, Nature Communications, 8, 1330 (2017)
7. Eun-Kyung Lim, Vasyl Yurchyshyn1, Pankaj Kumar1, Kyuhyoun Cho, Chaowei Jiang, Sujin Kim, Heesu Yang, Jongchul Chae, Kyung-Suk Cho, and Jeongwoo Lee, Observation of a Large-scale Quasi-circular Secondary Ribbon Associated with Successive Flares and a Halo CME, The Astrophysical Journal, 850, 167 (2017)

2017年以前
1. Jiang, C. W., Wu, S. T., Yurchyshyn, V., Wang, H. M., Feng, X. S., Hu, Q., How Did a Major Confined Flare Occur in Super Solar Active Region 12192?, The Astrophysical Journal, 828, 62 (2016)
2. Jiang, C. W., Wu, S. T., Feng, X., & Hu, Q., Data-driven Magnetohydrodynamic Modelling of a Flux-emerging Active Region Leading to Solar Eruption. Nature Communications, 7, 11522 (2016)
3. Jiang, C. W., Wu, S. T., and Feng, X., Analyses of the Photospheric Magnetic Dynamics in Solar Active Region 11117 Using an Advanced CESE-MHD Model, Front. Astron. Space Sci. 3, 16 (2016)
4. Jiang, C. W., Wu, S. T., Feng, X. S., Hu, Q., A Comparison Study of a Solar Active-Region Eruptive Filament and a Neighboring Non-Eruptive Filament, Research in Astronomy and Astrophysics, 16, 18 (2016)
5. Jiang, C. W., Feng, X. S., Testing a Solar Coronal Magnetic Field Extrapolation Code with the Titov-Demoulin Magnetic Flux Rope Model, Research in Astronomy and Astrophysics, 16, 15 (2016)
6. Jiang, C. W., Wu, S. T., Feng, X. S., Hu, Q., Nonlinear Force-free Field Extrapolation of a Coronal Magnetic Flux Rope Supporting a Large-scale Solar Filament from a Photospheric Vector Magnetogram, The Astrophysical Journal Letters, 786, L16 (2014)
7. Jiang, C. W., Wu, S. T., Feng, X. S., Hu, Q., Formation and Eruption of an Active Region Sigmoid. I. a Study by Nonlinear Force-Free Field Modeling, The Astrophysical Journal, 780, 55 (2014)
8. Jiang, C. W., Feng, X. S., Preprocessing the Photospheric Vector Magnetograms for an NLFFF Extrapolation Using a Potential-Field Model and an Optimization Method, Solar Physics, 289, 63 (2014)
9. Jiang, C. W., Feng, X. S., Wu, S. T., Hu, Q., Magnetohydrodynamic Simulation of a Sigmoid Eruption of Active Region 11283, The Astrophysical Journal Letters, 771, L30 (2013)
10. Jiang, C. W., Feng, X. S. Extrapolation of the Solar Coronal Magnetic Field From SDO/HMI Magnetogram using a CESE–MHD–NLFFF Code, The Astrophysical Journal, 769, 144 (2013)
11. Jiang, C. W., Feng, X. S., S. T. Wu, and Hu, Q., Study of The Three-Dimensional Coronal Magnetic Field of AR 11117 Around The Time of A Confined Flare Using A Data-Driven CESE-MHD Model, The Astrophysical Journal, 759, 85 (2012)
12. Jiang, C. W., Feng, X. S., A New Implementation of the MHD-Relaxation Method for Nonlinear Force-Free Field Extrapolation in the Solar Corona, The Astrophysical Journal, 749, 135 (2012)
13. Jiang, C. W., Feng, X. S., and Xiang, C. Q., A New Code For Nonlinear Force-Free Field Extrapolation Of The Global Corona, The Astrophysical Journal, 755, 62 (2012)
14. Jiang, C. W. and Feng, X. S., A Unified and Very Fast Way for Computing the Global Potential and Linear Force-Free Fields, Solar Physics, 281, 621 (2012)
15. Jiang, C. W., Cui S. X., Feng, X. S., Solving the Euler and Navier Stokes Equations by the AMR CESE method, Computers & Fluids, 54, 105 (2012)
16. Jiang, C. W., Feng, X. S., Fan, Y. L., Xiang, C. Q., Reconstruction of the Coronal magnetic field using the CESE-MHD method, The Astrophysical Journal, 727, 101 (2011)
17. Jiang, C. W., Feng, X. S., Zhang, J., Zhong, D. K., AMR Simulations of MHD Problems by the CESE Method in Curvilinear Coordinates, Solar Physics, 267, 463 (2010)
18. Wu, S. T., Zhou, Y., Jiang, C. W., Feng, X., Wu, C.-C., and Hu, Q., A data-constrained three-dimensional magnetohydrodynamic simulation model for a coronal mass ejection initiation, J. Geophys. Res. Space Physics, 121, 1009 (2016)
19. Sun, L. C., Xu, J. Y., Wang, W. B., Yuan, W., Li, Q. Z., and Jiang, C. W., A statistical analysis of equatorial plasma bubble structures based on an all-sky airglow imager network in China, Journal of Geophysical Research-Space Physics, 121, 11495 (2016)
20. Liu, C., Deng, N., Lee, J., Wiegelmann, T., Jiang, C., Dennis, B. R., Su, Y., Donea, A., and Wang, H., Three-dimensional Magnetic Restructuring in Two Homologous Solar Flares in the Seismically Active NOAA AR 11283, The Astrophysical Journal, 795, 128 (2014)
21. Zhang, J., Yang, S. H., Li, T., Jiang, C. W., Magnetic Reconnection: From “Open” Extreme-Ultraviolet Loops to Closed Post-Flare Ones Observed by SDO, The Astrophysical Journal, 776, 57 (2013)
22. Zhang, J., Zhang, L., Jiang, C. W., A Parallel Overlapping Curvilinear AMR Grids Management Tool Based on PARAMESH, Procedia Engineering, 61, 233 (2013)
23. Feng, X. S., Jiang, C. W., Xiang, C. Q., Zhao, X. P., and S. T. Wu., A Data-Driven Model For The Global Coronal Evolution, The Astrophysical Journal, 758, 62 (2012)
24. Feng, X. S., Yang, L. P., Xiang, C. Q., Jiang, C. W., Ma, X. P., Wu, S. T., Zhong, D. K., Zhou, Y. F. Validation of the 3D AMR SIP–CESE Solar Wind Model for Four Carrington Rotations, Solar Physics, 279, 207 (2012)
25. Zhang, Y. Y., Feng, X. S., Jiang, C. W., Zhou, Y. F., The Application of ADER Scheme in MHD Simulation, Chin. J. Space Sci., 32, 170-181 (2012)
26. Zhao X. H., S. T. Wu, A. H. Wang, A. Vourlidas, X. S. Feng, and Jiang, C. W., Uncovering the Wave Nature of the EUV Wave for the 2010 January 17 Event Through Its Correlation to the Background Magnetosonic Speed, The Astrophysical Journal, 742, 131 (2011)
27. Feng, X. S., Zhang, S. H., Xiang, C. Q., Yang, L. P., Jiang, C. W., and S. T. Wu, A hybrid solar wind model of the CESE+HLL method with a yin-yang overset grid and an AMR grid, The Astrophysical Journal, 734, 50 (2011)
28. Yang, L., Feng, X. S., Xiang, C. Q., Jiang, C. W., Numerical Validation and Comparison of Three Solar Wind Heating Methods by the SIP-CESE MHD Model, Chin. Phys. Lett. 28, 3 (2011)
会议论文及发表演说
2019年
参加第二届中欧太阳物理会议（克罗地亚，5月），做口头报告《Data-Driven MHD Simulation of Solar Eruptions》，并展示Poster《MHD Simulation of the X9.3 Flare on 2017 September 6》。
参加 ISSI-BJ Team \