Publications of Fang Shen

A list of publications authored or co-authored by Fang Shen, derived from the SAO/NASA Astrophysics Data System (ADS). The number in brackets after each title indicates the number of citations that the paper has received.

Orcid ID: 0000-0002-4935-6679

List of publications ordered by citations
Number of papers: 55 (refereed: 55)
No. of citations: 966
First author papers: 15 (refereed: 15)

2025

  1. Automatic 3D Reconstruction of Coronal Mass Ejections Based on Dual-viewpoint Observations and Machine Learning [0]
    Lin, Rongpei, Yang, Yi, Shen, Fang, Pi, Gilbert & Li, Yucong, ApJS, 280, 44
  2. Modeling Energetic Proton Transport from a Stream Interaction Region to Compound Streams [0]
    Tao, Xinyi, Shen, Fang & Luo, Xi, ApJ, 978, 143
  3. Natural Generation of Alfvén Waves from Three-dimensional Bursty Interchange Magnetic Reconnection in the Solar Corona [4]
    Yang, Liping, He, Jiansen, Feng, Xueshang, Verscharen, Daniel, Guo, Fan, Li, Hui, Tian, Hui, Li, Wenya, Shen, Fang, Hou, Chuanpeng, Shi, Mijie, Wu, Honghong & Xiong, Ming, ApJ, 982, L25
  4. Expansion-induced Three-part Morphology of the 2021 December 4 Coronal Mass Ejection [2]
    Yang, Liping, Feng, Xueshang, Shen, Fang, Xiong, Ming, Shen, Chenglong, Chi, Yutian, Wang, Yuming, Yan, Kuo, Ma, Mengxuan, Zhou, Yufen, Zhang, Man & Zhao, Xinhua, ApJ, 981, 109

2024

  1. CME Arrival Time Prediction Based on Coronagraph Observations and Machine-learning Techniques [3]
    Li, Yucong, Yang, Yi, Shen, Fang, Tang, Bofeng & Lin, Rongpei, ApJ, 976, 141
  2. An Algorithm for the Determination of Coronal Mass Ejection Kinematic Parameters Based on Machine Learning [3]
    Lin, Rongpei, Yang, Yi, Shen, Fang, Pi, Gilbert & Li, Yucong, ApJS, 271, 59
  3. A Numerical Study of the Effects of a Corotating Interaction Region on Cosmic-Ray Transport. II. Features of Cosmic-Ray Composition and Rigidity [5]
    Luo, Xi, Potgieter, Marius S., Zhang, Ming & Shen, Fang, ApJ, 961, 21
  4. Interplanetary Rotation of 2021 December 4 Coronal Mass Ejection on Its Journey to Mars [3]
    Ma, Mengxuan, Yang, Liping, Shen, Fang, Shen, Chenglong, Chi, Yutian, Wang, Yuming, Zhou, Yufen, Zhang, Man, Heyner, Daniel, Auster, Uli, Richter, Ingo & Sanchez-Cano, Beatriz, ApJ, 976, 183
  5. Modeling energetic proton transport in a corotating interaction region. An energetic particle event observed by STEREO-A from 21 to 24 August 2016 [1]
    Tao, Xinyi, Shen, Fang, Wei, Wenwen, Zhu, Yuji, Luo, Xi & Feng, XueShang, A&A, 682, A82
  6. Magnetohydrodynamic Modeling of Background Solar Wind near Mars: Comparison with MAVEN and Tianwen-1 [2]
    Zhang, Hanke, Shen, Fang, Yang, Yi, Chi, Yutian, Shen, Chenglong & Tao, Xinyi, ApJ, 971, 151
  7. Solar Energetic Particles Propagation under 3D Corotating Interaction Regions with Different Characteristic Parameters [0]
    Zhu, Yuji & Shen, Fang, Universe, 10, 315

2023

  1. Reconstructing Synoptic Maps of Solar Wind Radial Velocity between 20 and 60 R ⊙ Based on STEREO/HI1 Images [2]
    Li, Xiaolei, Wang, Yuming, Shen, Fang, Yang, Yi, Zhang, Quanhao & Lyu, Shaoyu, ApJ, 949, 58
  2. A New Numerical Implementation for Solar Coronal Modeling by an HLL Generalized Riemann Problem Solver [0]
    Liu, Mengqing, Zhang, Man, Liu, Xiaojing & Shen, Fang, ApJS, 264, 25
  3. Global Morphology Distortion of the 2021 October 9 Coronal Mass Ejection from an Ellipsoid to a Concave Shape [9]
    Yang, Liping, Hou, Chuanpeng, Feng, Xueshang, He, Jiansen, Xiong, Ming, Zhang, Man, Zhou, Yufen, Shen, Fang, Zhao, Xinhua, Li, Huichao, Yang, Yi & Liu, Xiaojing, ApJ, 942, 65
  4. Research on the Effect of Data Assimilation for Three-Dimensional MHD Simulation of Solar Wind [2]
    Zhang, Hanke, Shen, Fang & Yang, Yi, Space Weather, 21, e2023SW003429

2022

  1. Numerical Research on the Effect of the Initial Parameters of CME Flux-rope Model on Simulation Results. III. Different Initial Energy of CMEs [2]
    Liu, Yousheng, Shen, Fang, Yang, Yi & Ma, Mengxuan, ApJ, 940, 11
  2. Propagation characteristics of coronal mass ejections (CMEs) in the corona and interplanetary space [23]
    Shen, Fang, Shen, Chenglong, Xu, Mengjiao, Liu, Yousheng, Feng, Xueshang & Wang, Yuming, Reviews of Modern Plasma Physics, 6, 8
  3. Implicit Solar Coronal Magnetohydrodynamic (MHD) Modeling with a Low-dissipation Hybridized AUSM-HLL Riemann Solver [6]
    Wang, Haopeng, Xiang, Changqing, Liu, Xiaojing, Lv, Jiakun & Shen, Fang, ApJ, 935, 46
  4. Energy Spectra Variations of Energetic Ions Associated With a Stream Interaction Region [3]
    Wei, Wenwen, Zhuang, Bin, Huang, Jia, Shen, Fang, Zhao, Lulu, Liu, Mingzhe, Zhang, Xiaoxin & Feng, Xueshang, Journal of Geophysical Research (Space Physics), 127, e2022JA030652

2021

  1. Magnetohydrodynamic Modeling of the Solar Corona with an Effective Implicit Strategy [16]
    Feng, Xueshang, Wang, Haopeng, Xiang, Changqing, Liu, Xiaojing, Zhang, Man, Zhao, Jingmin & Shen, Fang, ApJS, 257, 34
  2. A new locally divergence-free WLS-ENO scheme based on the positivity-preserving finite volume method for ideal MHD equations [8]
    Liu, Mengqing, Zhang, Man, Li, Caixia & Shen, Fang, Journal of Computational Physics, 447, 110694
  3. Numerical Research on the Effect of the Initial Parameters of a CME Flux-rope Model on Simulation Results [17]
    Shen, Fang, Liu, Yousheng & Yang, Yi, ApJS, 253, 12
  4. Numerical Research on the Effect of the Initial Parameters of a CME Flux-rope Model on Simulation Results. II. Different Locations of Observers [6]
    Shen, Fang, Liu, Yousheng & Yang, Yi, ApJ, 915, 30
  5. Numerical MHD Simulations of the 3D Morphology and Kinematics of the 2017 September 10 CME-driven Shock from the Sun to Earth [13]
    Yang, Liping, Wang, Haopeng, Feng, Xueshang, Xiong, Ming, Zhang, Man, Zhu, Bei, Li, Huichao, Zhou, Yufen, Shen, Fang, Zhao, Xinhua & Liu, Xiaojing, ApJ, 918, 31
  6. Numerical Study of Two Injection Methods for the 2007 November 15 Coronal Mass Ejection in the Inner Heliosphere [2]
    Zhang, Man, Feng, Xueshang, Shen, Fang & Yang, Liping, ApJ, 918, 35

2020

  1. Reconstructing Solar Wind Inhomogeneous Structures From Stereoscopic Observations in White Light: Solar Wind Transients in 3-D [11]
    Li, Xiaolei, Wang, Yuming, Liu, Rui, Shen, Chenglong, Zhang, Quanhao, Lyu, Shaoyu, Zhuang, Bin, Shen, Fang, Liu, Jiajia & Chi, Yutian, Journal of Geophysical Research (Space Physics), 125, e27513
  2. A Numerical Study of the Effects of Corotating Interaction Regions on Cosmic-Ray Transport [22]
    Luo, Xi, Zhang, Ming, Feng, Xueshang, Potgieter, Marius S., Shen, Fang & Bazilevskaya, Galina, ApJ, 899, 90
  3. MHD Modeling of the Background Solar Wind in the Inner Heliosphere From 0.1 to 5.5 AU: Comparison With In Situ Observations [9]
    Wang, Y. X., Guo, X. C., Wang, C., Florinski, V., Shen, F., Li, H. & Blanc, M., Space Weather, 18, e02262

2019

  1. Hyperbolic Cell-centered Finite Volume Method for Obtaining Potential Magnetic Field Solutions [3]
    Liu, Xiaojing, Feng, Xueshang, Xiang, Changqing & Shen, Fang, ApJ, 887, 33
  2. Numerical Simulation on the Propagation and Deflection of Fast Coronal Mass Ejections (CMEs) Interacting with a Corotating Interaction Region in Interplanetary Space [35]
    Liu, Yousheng, Shen, Fang & Yang, Yi, ApJ, 887, 150
  3. Modeling solar energetic particle transport in 3D background solar wind: Influences of the compression regions [16]
    Wei, Wenwen, Shen, Fang, Yang, Zicai, Zhao, Lulu, Wang, Yang, Zuo, Pingbing & Zhang, Jie, Journal of Atmospheric and Solar-Terrestrial Physics, 182, 155
  4. Modeling the Global Distribution of Solar Wind Parameters on the Source Surface Using Multiple Observations and the Artificial Neural Network Technique [9]
    Yang, Yi & Shen, Fang, Solar Physics, 294, 111

2018

  1. Three-dimensional MHD Simulation of Solar Wind Using a New Boundary Treatment: Comparison with In Situ Data at Earth [47]
    Shen, Fang, Yang, Zicai, Zhang, Jie, Wei, Wenwen & Feng, Xueshang, ApJ, 866, 18
  2. Prediction of Solar Wind Speed at 1 AU Using an Artificial Neural Network [46]
    Yang, Yi, Shen, Fang, Yang, Zicai & Feng, Xueshang, Space Weather, 16, 1227
  3. Correlation Between the Magnetic Field and Plasma Parameters at 1 AU [7]
    Yang, Zicai, Shen, Fang, Zhang, Jie, Yang, Yi, Feng, Xueshang & Richardson, Ian G., Solar Physics, 293, 24

2017

  1. On the Collision Nature of Two Coronal Mass Ejections: A Review [32]
    Shen, Fang, Wang, Yuming, Shen, Chenglong & Feng, Xueshang, Solar Physics, 292, 104

2016

  1. Turn on the super-elastic collision nature of coronal mass ejections through low approaching speed [19]
    Shen, Fang, Wang, Yuming, Shen, Chenglong & Feng, Xueshang, Scientific Reports, 6, 19576
  2. On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015 [41]
    Wang, Yuming, Zhang, Quanhao, Liu, Jiajia, Shen, Chenglong, Shen, Fang, Yang, Zicai, Zic, T., Vrsnak, B., Webb, D. F., Liu, Rui, Wang, S., Zhang, Jie, Hu, Qiang & Zhuang, Bin, Journal of Geophysical Research (Space Physics), 121, 7423

2015

  1. Why Does the Apparent Mass of a Coronal Mass Ejection Increase? [33]
    Feng, Li, Wang, Yuming, Shen, Fang, Shen, Chenglong, Inhester, Bernd, Lu, Lei & Gan, Weiqun, ApJ, 812, 70

2014

  1. Evolution of the 12 July 2012 CME from the Sun to the Earth: Data-constrained three-dimensional MHD simulations [79]
    Shen, Fang, Shen, Chenglong, Zhang, Jie, Hess, Phillip, Wang, Yuming, Feng, Xueshang, Cheng, Hongze & Yang, Yi, Journal of Geophysical Research (Space Physics), 119, 7128
  2. Deflected propagation of a coronal mass ejection from the corona to interplanetary space [100]
    Wang, Yuming, Wang, Boyi, Shen, Chenglong, Shen, Fang & Lugaz, Noé, Journal of Geophysical Research (Space Physics), 119, 5117

2013

  1. Could the collision of CMEs in the heliosphere be super−elastic? Validation through three−dimensional simulations [52]
    Shen, Fang, Shen, Chenglong, Wang, Yuming, Feng, Xueshang & Xiang, Changqing, Geophysical Research Letters, 40, 1457

2012

  1. Acceleration and deceleration of coronal mass ejections during propagation and interaction [52]
    Shen, Fang, Wu, S. T., Feng, Xueshang & Wu, Chin-Chun, Journal of Geophysical Research (Space Physics), 117, A11101
  2. Improvement to the global distribution of coronal plasma and magnetic field on the source surface using expansion factor fs and angular distance θb [8]
    Shen, Fang, Feng, Xueshang & Xiang, Changqing, Journal of Atmospheric and Solar-Terrestrial Physics, 77, 125
  3. Using a 3-D spherical plasmoid to interpret the Sun-to-Earth propagation of the 4 November 1997 coronal mass ejection event [36]
    Zhou, Y. F., Feng, X. S., Wu, S. T., Du, D., Shen, F. & Xiang, C. Q., Journal of Geophysical Research (Space Physics), 117, A01102

2011

  1. Energy transfer during intense geomagnetic storms driven by interplanetary coronal mass ejections and their sheath regions [57]
    Guo, Jianpeng, Feng, Xueshang, Emery, Barbara A., Zhang, Jie, Xiang, Changqing, Shen, Fang & Song, Wenbin, Journal of Geophysical Research (Space Physics), 116, A05106
  2. Three-dimensional MHD simulation of the evolution of the April 2000 CME event and its induced shocks using a magnetized plasma blob model [37]
    Shen, F., Feng, X. S., Wu, S. T., Xiang, C. Q. & Song, W. B., Journal of Geophysical Research (Space Physics), 116, A04102
  3. Differential Rotation of Strong Magnetic Flux During Solar Cycles 21 - 23 [3]
    Song, W. B., Feng, X. S., Shen, F. & Guo, J. P., Solar Physics, 270, 35

2010

  1. The statistical and numerical study of the global distribution of coronal plasma and magnetic field near 2.5 Rs over a 10-year period [11]
    Shen, Fang, Feng, Xueshang, Xiang, Changqing & Song, Wenbin, Journal of Atmospheric and Solar-Terrestrial Physics, 72, 1008
  2. The heating of the solar transition region [2]
    Song, Wen-Bin, Feng, Xue-Shang & Shen, Fang, Research in Astronomy and Astrophysics, 10, 529

2009

  1. The theoretical research of basic function method in incompressible viscous flow and its simulations in three-dimensional aneurysms [0]
    Shen, Fang & Wu, Wangyi, Science in China: Physics, Mechanics and Astronomy, 52, 909
  2. An asynchronous and parallel time-marching method: Application to three-dimensional MHD simulation of solar wind [18]
    Shen, Fang, Feng, XueShang & Song, WenBin, Science in China E: Technological Sciences, 52, 2895
  3. Variability of Extended Bipolar Regions [2]
    Song, W. B., Feng, X. S., Shen, F. & Zhang, Y. Z., Solar Physics, 257, 83

2008

  1. A solar eruption triggered by merge interactions of different helicity loops [2]
    Song, W., Feng, X. & Shen, F., A&A, 485, L13

2007

  1. Three-dimensional MHD simulation of CMEs in three-dimensional background solar wind with the self-consistent structure on the source surface as input: Numerical simulation of the January 1997 Sun-Earth connection event [45]
    Shen, Fang, Feng, Xueshang, Wu, S. T. & Xiang, Changqing, Journal of Geophysical Research (Space Physics), 112, A06109

Created on Sat Nov 22 04:32:35 2025.