2010

1. Xueshang Feng, Liping Yang, Changqing Xiang, S. T. Wu, Yufen Zhou and DingKun Zhong, THREE-DIMENSIONAL SOLAR WIND MODELING FROM THE SUN TO EARTH BY A SIP-CESE MHD MODEL WITH A SIX-COMPONENT GRID, 2010 ApJ 723 300, doi:10.1088/0004-637X/723/1/300. [pdf]

2. Guo, J., X. Feng, J. M. Forbes, J. Lei, J. Zhang, and C. Tan (2010), On the relationship between thermosphere density and solar wind parameters during intense geomagnetic storms, J. Geophys. Res., 115, A12335, doi:10.1029/2010JA015971. [pdf]

3. Zuo, P. B., F. S. Wei, X. S. Feng, X. J. Xu, and W. B. Song (2010), Magnetic cloud boundary layer of 9 November 2004 and its associated space weather effects, J. Geophys. Res., 115, A10102, doi:10.1029/2009JA014815. [pdf]

4. Song W.B., X. Feng and F. Shen (2010), The heating of the solar transition region, Research in Astron. Astrophys. Vol. 10 No. 6, 529–532. [pdf]

5. Guo, J., et al., Interplanetary drivers of ionospheric prompt penetration electric fields. Journal of Atmospheric and Solar-Terrestrial Physics(2010), doi:10.1016/j.jastp.2010.01.010. [pdf]

6. Guo, J., X. Feng, J. Zhang, P. Zuo, and C. Xiang (2010), Statistical properties and geoefficiency of interplanetary coronal mass ejections and their sheaths during intense geomagnetic storms, J. Geophys. Res., 115, A09107, doi:10.1029/2009JA015140. [pdf]

7. Shen F., X. Feng, C. Xiang,W. Song (2010), The statistical and numerical study of the global distribution of coronal plasma and magnetic field near 2.5 Rs over a 10-year period, Journal of Atmospheric and Solar-Terrestrial Physics 72:1008–1018, doi:10.1016/j.jastp.2010.05.016. [pdf]

8. Zhang Y, Chen J Y, Feng X S(2010), Predicting the shock arrival time using 1D-HD solar wind model. Chinese Sci Bull, 2010, 55: 1053-1058, doi: 10.1007/s11434-009-0610-8. [pdf]

9. Zhao, X. H., X. S. Feng, C. Q. Xiang, Y. Liu, Z. Li, Y. Zhang, and S. T. Wu(2010), Multi-spacecraft observations of the 2008 January 2 CME in the inner heliosphere,The Astrophysical Journal, 714:1133–1141, doi:10.1088/0004-637X/714/2/1133. [pdf]

10. Song, W.B.(2010), An Analytical Model to Predict the Arrival Time of Interplanetary CMEs, Solar Phys 261: 311–320, DOI 10.1007/s11207-009-9486-7. [pdf]

11. Wang Y., F. S. Wei, X. S. Feng, S. H. Zhang, P. B. Zuo,1 and T. R. Sun(2010), Energetic Electrons Associated with Magnetic Reconnection in the Magnetic Cloud Boundary Layer, PHYSICAL REVIEW LETTERS (2010) PRL 105, 195007, DOI: 10.1103/PhysRevLett.105.195007. [pdf]

12. Li, Z., F.S. Wei, X.S. Feng, X.H. Zhao(2010), The “Same Side –Opposite Side Effect” of the Heliospheric Current Sheet in Ionospheric Negative Storms, Solar Phys (2010) 263: 263–273, DOI 10.1007/s11207-010-9559-7. [pdf]

13. Jiang, Feng, Zhang, and Zhong, AMR Simulations of magnetohydrodynamic Problems By the CESE Method In Curvilinear Coordinates,Solar physics,2010, 267: 463-491,  DOI 10.1007/s11207-010-9649-6. [pdf]

14. Jizhen,Zhou Yufeng, A Comparison Study of Three CESE Schemes in MHD Simulation, CHIN. PHYS. LETT. Vol. 27, No. 8 (2010) 085201.[pdf]

15. 刘元昕,纪珍,电阻磁流体力学的CESE方法,空间科学学报,2010, 30(3): 211-220. [pdf]

16. 张莹 冯学尚 杨利平,运用一维太阳风MHD CE/SE模型预报行星际激波到达时间,空间科学学报,2010 30(2), 2010, 30(2): 105-112. [pdf]

17. Zhao Xinhua, Xiang Changqing. Advance of interplanetary physics study in China: 2008–2010. Chinese Journal of Space Science, 2010, 30(5) : 427-444. [pdf]