1. Li Z, Wei FS, Feng XS, Guo JP, Emery BA, Zhao XH, Large ionospheric disturbances during a minor geomagnetic storm on June 23, 2000, ANNALS OF GEOPHYSICS, 55(2):253-263, 2012, doi: 10.4401/ag-5409. [pdf]

2. Zhang Shaohua, Feng Xueshang, Yang Liping, 2.5D AMR MHD magnetic reconnection model, Chin. J. Space Sci., 2012, 32(6): 785-792. [pdf]

3. Xu Xiaojun, Wei Fengsi, Feng Xueshang, Characteristics of reconnection diffusion region in the solar wind, Chin. J. Space Sci., 2012, 32(6): 778-784. [pdf]

4. Fang Shen, Xueshang Feng, and S. T. Wu, 3D MHD Numerical Study of Two CMEs' Evolution and Their Interaction, Astronomical Society of the Pacific Conference Series, Vol. 459, 247-252. [pdf]

5. S. T. Wu, A. H. Wang, David Falconer, Qiang Hu, Yang Liu, Xueshang Feng, and Fang Shen, Modeling of Solar Active Region Using a Three-Dimensional, Time-Dependent, Data-Driven Magnetohydrodynamic Model, Astronomical Society of the Pacific Conference Series,  Vol. 459, 247-252. [pdf]

6. Feng, X.; Yang, L. P.; Xiang, C. Q.; Liu, Y.; Zhao, X.; Wu, S. T., Numerical Study of the Global Corona for CR 2055 Driven by Daily Updated Synoptic Magnetic Field , Numerical Modeling of Space Plasma Slows (ASTRONUM 2011), Astronomical Society of the Pacific Conference Series, , Vol. 459, 202-208. [pdf]

7. Zhao Xinhua, Xiang Changqing, Research progress of solar corona and interplanetary physics in China: 2010−2012, Chin. J. Space Sci., 2012, 32(5): 618-646, doi: 0254-6124/2012/32(5)-618–29. [pdf]

8. Xueshang Feng, Chaowei Jiang, Changqing Xiang, Xuepu Zhao, and S. T. Wu (2012), A DATA-DRIVEN MODEL FOR THE GLOBAL CORONAL EVOLUTION, The Astrophysical Journal, 758:62 (13pp), 2012, doi: 10.1088/0004-637X/758/1/62. [pdf]

9. Chaowei Jiang, Xueshang Feng, S. T. Wu, and Qiang Hu (2012), Study of the Three-dimensional Coronal Magnetic Field of Active Region 11117 around the Time of a Confined Flare Using a Data-Driven CESE-MHD Model, The Astrophysical Journal, 759 85, doi: 10.1088/0004-637X/759/2/85. [pdf]

10. Shen, F., S. T. Wu, X. Feng, and C.-C. Wu (2012), Acceleration and deceleration of coronal mass ejections during propagation and interaction, J. Geophys. Res., 117, A11101, doi: 10.1029/2012JA017776. [pdf]

11. Chaowei Jiang and Xueshang Feng (2012), A Unified and Very Fast Way for Computing the Global Potential and Linear Force-Free Fields, Solar Physics, 281(2), 621-637, doi: 10.1007/s11207-012-0074-x.[pdf]

12. Yang, L. P., X. S. Feng, C. Q. Xiang, Y. Liu, X. Zhao, and S. T. Wu (2012), Time-dependent MHD modeling of the global solar corona for year 2007: Driven by daily-updated magnetic field synoptic data, J. Geophys. Res., 117, A08110, doi: 10.1029/2011JA017494. [pdf]

13. Chaowei Jiang, Xueshang Feng, and Changqing Xiang, A NEW CODE FOR NONLINEAR FORCE-FREE FIELD EXTRAPOLATION OF THE GLOBAL CORONA, The Astrophysical Journal, 755:62 (13pp), 2012, doi: 10.1088/0004-637X/755/1/62. [pdf]

14. Zhou Y. F., X. S. Feng, A New Hybrid Numerical Scheme for Two-Dimensional Ideal MHD Equations, CHIN. PHYS. LETT. Vol. 29, No. 9 (2012) 094703, doi: 10.1088/0256-307X/29/9/094703. [pdf]

15. Li Zheng, Wei Fengsi, Feng Xueshang, Guo Jianpeng, Xu Xiaojun, A prediction method for Δf0F2min of a single station from interplanetary parameters based on statistical study, Chin. J. Space Sci., 2012, 32(3): 312-320.[pdf]

16. Hou Tianxiang, Ji Zhen, Modified two dimensional third-order semi-discrete central-upwind scheme, Chin. J. Space Sci., 2012, 32(2): 197-203. [pdf]

17. Zhang Yanyan, Feng Xueshang, Jiang Chaowei, Zhou Yufen, Application of ADER scheme in MHD simulation, Chin. J. Space Sci., 2012, 32(2): 170-181.[pdf]

18. Guo, J., X. Feng, B. A. Emery, and Y. Wang (2012), Efficiency of solar wind energy coupling to the ionosphere, J. Geophys. Res., 117, A07303, doi: 10.1029/2012JA017627. [pdf]

19. Feng S. W. , Y. Chen, X. L. Kong, G. Li, H. Q. Song, X. S. Feng, and Ying Liu, RADIO SIGNATURES OF CORONAL-MASS-EJECTION–STREAMER INTERACTION AND SOURCE DIAGNOSTICS OF TYPE II RADIO BURST, ApJ, 753, 21, doi: 10.1088/0004-637X/753/1/21. [pdf]

20. Xueshang Feng, Liping Yang, Changqing Xiang, Caowei Jiang, Xiaopeng Ma, S.T. Wu, DingKun Zhong and Yufen Zhou, Validation of the 3D AMR SIP–CESE SolarWind Model for Four Carrington Rotations, Solar Phys (2012) 279:207–229, doi: 10.1007/s11207-012-9969-9. [pdf]

21. Guo, J., X. Feng, T. I. Pulkkinen, E. I. Tanskanen, W. Xu, J. Lei, and B. A. Emery (2012), Auroral electrojets variations caused by recurrent high-speed solar wind streams during the extreme solar minimum of 2008, J. Geophys. Res., 117, A04307, doi: 10.1029/2011JA017458. [pdf]

22. Y. Wang and F. S. Wei and X. S. Feng and P. B. Zuo and J. P. Guo and X. J. Xu and Z. Li, Variations of Solar Electron and Proton Flux in Magnetic Cloud Boundary Layers and Comparisons with Those across the Shocks and in the Reconnection Exhausts, The Astrophysical Journal, 749:82 (10pp), 2012, doi: 10.1088/0004-637X/749/1/82. [pdf]

23. Chaowei Jiang and Xueshang Feng, A NEW IMPLEMENTATION OF THE MAGNETOHYDRODYNAMICS-RELAXATION METHOD FOR NONLINEAR FORCE-FREE FIELD EXTRAPOLATION IN THE SOLAR CORONA, The Astrophysical Journal,749:135 (19pp), 2012, doi: 10.1088/0004-637X/749/2/135. [pdf]

24. Fang Shen, Xueshang Feng, Changqing Xiang, Improvement to the global distribution of coronal plasma and magnetic field on the source surface using expansion factor fs and angular distance, Journal of Atmospheric and Solar-Terrestrial Physics 77 (2012) 125–131, doi: 10.1016/j.jastp.2011.12.009. [pdf]

25. Zhou, Y. F., X. S. Feng, S. T. Wu, D. Du, F. Shen, and C. Q. Xiang (2012), Using a 3-D spherical plasmoid to interpret the Sun-to-Earth propagation of the 4 November 1997 coronal mass ejection event, J. Geophys. Res., 117, A01102, doi: 10.1029/2010JA016380. [pdf]

26. Chaowei Jiang, Shuxin Cui, Xueshang Feng, Solving the Euler and Navier Stokes equations by the AMR CESE method, Computers & Fluids, 54 (2012) 105 117, doi: 10.1016/j.compfluid.2011.10.006. [pdf]