| Deflection of coronal mass ejection in the interplanetary medium Y Wang, C Shen, S Wang, P Ye Solar Physics 222, 329-343, 2004 | 142 | 2004 |
| Why is the great solar active region 12192 flare-rich but CME-poor? X Sun, MG Bobra, JT Hoeksema, Y Liu, Y Li, C Shen, S Couvidat, ... The Astrophysical Journal Letters 804 (2), L28, 2015 | 135 | 2015 |
| Energetic electron distributions fitted with a relativistic kappa‐type function at geosynchronous orbit F Xiao, C Shen, Y Wang, H Zheng, S Wang Journal of Geophysical Research: Space Physics 113 (A5), 2008 | 129 | 2008 |
| Quantitative analysis of CME deflections in the corona B Gui, C Shen, Y Wang, P Ye, J Liu, S Wang, X Zhao Solar Physics 271, 111-139, 2011 | 119 | 2011 |
| Kinematic evolution of a slow CME in corona viewed by STEREO-B on 8 October 2007 C Shen, Y Wang, B Gui, P Ye, S Wang Solar Physics 269, 389-400, 2011 | 114 | 2011 |
| Super-elastic collision of large-scale magnetized plasmoids in the heliosphere C Shen, Y Wang, S Wang, Y Liu, R Liu, A Vourlidas, B Miao, P Ye, J Liu, ... Nature Physics 8 (12), 923-928, 2012 | 107 | 2012 |
| Statistical study of coronal mass ejection source locations: Understanding CMEs viewed in coronagraphs Y Wang, C Chen, B Gui, C Shen, P Ye, S Wang Journal of Geophysical Research: Space Physics 116 (A4), 2011 | 100 | 2011 |
| Evolution of the 12 July 2012 CME from the Sun to the Earth: Data‐constrained three‐dimensional MHD simulations F Shen, C Shen, J Zhang, P Hess, Y Wang, X Feng, H Cheng, Y Yang Journal of Geophysical Research: Space Physics 119 (9), 7128-7141, 2014 | 96 | 2014 |
| Statistical study of the interplanetary coronal mass ejections from 1995 to 2015 Y Chi, C Shen, Y Wang, M Xu, P Ye, S Wang Solar Physics 291, 2419-2439, 2016 | 95 | 2016 |
| Deflected propagation of a coronal mass ejection from the corona to interplanetary space Y Wang, B Wang, C Shen, F Shen, N Lugaz Journal of Geophysical Research: Space Physics 119 (7), 5117-5132, 2014 | 93 | 2014 |
| A new tool for CME arrival time prediction using machine learning algorithms: CAT-PUMA J Liu, Y Ye, C Shen, Y Wang, R Erdélyi The Astrophysical Journal 855 (2), 109, 2018 | 76 | 2018 |
| Why the shock-ICME complex structure is important: Learning from the early 2017 September CMEs C Shen, M Xu, Y Wang, Y Chi, B Luo The Astrophysical Journal 861 (1), 28, 2018 | 67 | 2018 |
| Buildup of a highly twisted magnetic flux rope during a solar eruption W Wang, R Liu, Y Wang, Q Hu, C Shen, C Jiang, C Zhu Nature communications 8 (1), 1330, 2017 | 66 | 2017 |
| An empirical formula relating the geomagnetic storm's intensity to the interplanetary parameters: − and Δt Y Wang, CL Shen, S Wang, PZ Ye Geophysical Research Letters 30 (20), 2003 | 65 | 2003 |
| Understanding the twist distribution inside magnetic flux ropes by anatomizing an interplanetary magnetic cloud Y Wang, C Shen, R Liu, J Liu, J Guo, X Li, M Xu, Q Hu, T Zhang Journal of Geophysical Research: Space Physics 123 (5), 3238-3261, 2018 | 63 | 2018 |
| Impact of major coronal mass ejections on geospace during 2005 September 7-13 Y Wang, X Xue, C Shen, P Ye, S Wang, J Zhang The Astrophysical Journal 646 (1), 625, 2006 | 61 | 2006 |
| On the twists of interplanetary magnetic flux ropes observed at 1 AU Y Wang, B Zhuang, Q Hu, R Liu, C Shen, Y Chi Journal of Geophysical Research: Space Physics 121 (10), 9316-9339, 2016 | 59 | 2016 |
| Could the collision of CMEs in the heliosphere be super‒elastic? Validation through three‒dimensional simulations F Shen, C Shen, Y Wang, X Feng, C Xiang Geophysical Research Letters 40 (8), 1457-1461, 2013 | 59 | 2013 |
| Why is a flare-rich active region CME-poor? L Liu, Y Wang, J Wang, C Shen, P Ye, R Liu, J Chen, Q Zhang, S Wang The Astrophysical Journal 826 (2), 119, 2016 | 58 | 2016 |
| Full‐halo coronal mass ejections: Arrival at the Earth C Shen, Y Wang, Z Pan, B Miao, P Ye, S Wang Journal of Geophysical Research: Space Physics 119 (7), 5107-5116, 2014 | 58 | 2014 |
Wang, YumingSchool of Earth and Space Sciences, University of Science and Technology of ChinaVerified email at ustc.edu.cn
