Chaowei Jiang-lnstitute of Space Science and Applied Technology

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Basic Information

Telephone: 0755－86249192
Address: Harbin Institute of Technology (Shenzhen) L818
E-mail: chaowei@hit.edu.cn
Research field: Coronal magnetic field extrapolations, Data-driven MHD simulation of Solar Eruption、Numerical model of Space weathe、High performance MHD numerical schemes.

Introducton

Chaowei Jiang received his B.S. in astronomy from Beijing Normal University in 2006, and Ph.D. in Space physics from University of Chinese Academy of Sciences in 2011. His research interests include reconstruction and analysis of solar magnetic fields, data-driven model of solar eruptions such as solar flares and coronal mass ejections, and advanced numerical techniques for space weather-related modeling. He has developed a suite of new high-accuracy and high-performance numerical codes for reconstruction of the 3D coronal fields, and further developed a data-driven MHD model that can realistically simulate the eruptive structures from their origin, formation until eruption. This provides a new, powerful way to reveal the long-standing puzzle of why and how solar eruption is produced. He has published more than 50 papers in top journals such as Nature Communications, The Astrophysical Journal, Astrophysical Journal Letters, which have been cited by over 1000 times. He won the BASU early career award in Sun-Earth Systems Science of American Geophysical Union in 2015.

Research Experience

2018-present professor, Harbin Institute of Technology (Shenzhen)
2017-2018 associate professor, Harbin Institute of Technology (Shenzhen)

2015-2016 Associate Researcher, the State Key Lab of Space Weather, Chinese Academy of Sciences

2013-2015 Postdoctor, Space Physics, University of Alabama in Huntsville

2011-2013 Postdoctor, Space Physics, the State Key Lab of Space Weather, Chinese Academy of Sciences

Education

2006-2011 PhD, Space Physics, University of Chinese Academy of Sciences

2002-2006 undergraduate, Astronomy, Beijing Normal University

Awards

Basu Early Career Award in Sun-Earth Systems Science, American Geophysical Union, 2015

the Excellent Doctoral Dissertation Award of Chinese Academy of Sciences，Chinese Academy of Sciences, 2013

Outstanding young scholars Thesis Award of the 8th National Space Weather Symposium, 2012

Selected as the 5th group member of the Youth Innovation Promotion Association of Chinese Academy of Sciences, Chinese Academy of Sciences, 2015

Teaching Courses

《Physics Lab IA，IB》

《the Physics of Solar Activities》

《Numerical Simulation of Space Weather》

Published Articles

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?, 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)