First-authored, refereed papers of Yao Chen
A list of first-authored, refereed publications of Yao Chen, 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: 0000-0001-6449-8838
List of publications ordered by citations
Number of papers: 23
No. of citations: 596
2022
- Plasma emission induced by ring-distributed energetic electrons in overdense plasmas [7]
Chen, Yao, Zhang, Zilong, Ni, Sulan, Ning, Hao, Li, Chuanyang & Li, Yaokun, Physics of Plasmas, 29, 112113
- Plasma Emission Induced by Electron Beams in Weakly Magnetized Plasmas [21]
Chen, Yao, Zhang, Zilong, Ni, Sulan, Li, Chuanyang, Ning, Hao & Kong, Xiangliang, ApJ, 924, L34
2017
- Double-coronal X-Ray and Microwave Sources Associated with a Magnetic Breakout Solar Eruption [24]
Chen, Yao, Wu, Zhao, Liu, Wei, Schwartz, Richard A., Zhao, Di, Wang, Bing & Du, Guohui, ApJ, 843, 8
2016
- Imaging a Magnetic-breakout Solar Eruption [60]
Chen, Yao, Du, Guohui, Zhao, Di, Wu, Zhao, Liu, Wei, Wang, Bing, Ruan, Guiping, Feng, Shiwei & Song, Hongqiang, ApJ, 820, L37
2014
- A Solar Type II Radio Burst from Coronal Mass Ejection-Coronal Ray Interaction: Simultaneous Radio and Extreme Ultraviolet Imaging [67]
Chen, Yao, Du, Guohui, Feng, Li, Feng, Shiwei, Kong, Xiangliang, Guo, Fan, Wang, Bing & Li, Gang, ApJ, 787, 59
2013
- A review of recent studies on coronal dynamics: Streamers, coronal mass ejections, and their interactions [23]
Chen, Yao, Chinese Science Bulletin, 58, 1599
2011
- A Coronal Seismological Study with Streamer Waves [56]
Chen, Y., Feng, S. W., Li, B., Song, H. Q., Xia, L. D., Kong, X. L. & Li, Xing, ApJ, 728, 147
2010
- Streamer Waves Driven by Coronal Mass Ejections [66]
Chen, Y., Song, H. Q., Li, B., Xia, L. D., Wu, Z., Fu, H. & Li, Xing, ApJ, 714, 644
2009
- Intrinsic Instability of Coronal Streamers [45]
Chen, Y., Li, X., Song, H. Q., Shi, Q. Q., Feng, S. W. & Xia, L. D., ApJ, 691, 1936
2007
- Catastrophic Eruption of Magnetic Flux Rope in the Corona and Solar Wind With and Without Magnetic Reconnection [43]
Chen, Y., Hu, Y. Q. & Sun, S. J., ApJ, 665, 1421
- Two energy release processes for CMEs: MHD catastrophe and magnetic reconnection [10]
Chen, Y., Hu, Y. Q. & Xia, L. D., Advances in Space Research, 40, 1780
2006
- Force Balance Analysis of a Coronal Magnetic Flux Rope in Equilibrium or Eruption [20]
Chen, Y., Li, G. Q. & Hu, Y. Q., ApJ, 649, 1093
- Catastrophe of Coronal Flux Rope in Unsheared and Sheared Bipolar Magnetic Fields [8]
Chen, Y., Chen, X. H. & Hu, Y. Q., ApJ, 644, 587
2005
- Velocity shear induced transition of magnetohydrodynamic to kinetic Alfvén waves [5]
Chen, Yao, Physics of Plasmas, 12, 052110
- Reproducing the UVCS/SOHO measurements in the slow wind source region at solar minimum [2]
Chen, Yao, Advances in Space Research, 36, 1461
2004
- An Ion-Cyclotron Resonance-driven Three-Fluid Model of the Slow Wind near the Sun [10]
Chen, Y. & Li, X., ApJ, 609, L41
- Stagnated Outflow of O+5 Ions in the Source Region of the Slow Solar Wind at Solar Minimum [18]
Chen, Y., Esser, R., Strachan, L. & Hu, Y., ApJ, 602, 415
2003
- Numerical modeling of the halo electrons in the fast solar wind [4]
Chen, Y., Esser, R. & Hu, Y. Q., Journal of Geophysical Research (Space Physics), 108, 1371
- Formation of Minor-Ion Charge States in the Fast Solar Wind: Roles of Differential Flow Speeds of Ions of the Same Element [34]
Chen, Y., Esser, R. & Hu, Y., ApJ, 582, 467
2002
- Effect of Flow-Tube Geometry on Solar Wind Properties [14]
Chen, Y. & Hu, Y. Q., Astrophysics and Space Science, 282, 447
- A theoretical model for O5+ (O7+) ions in the fast solar wind [4]
Chen, Yao, Esser, Ruth & Hu, You Qiu, Journal of Geophysical Research (Space Physics), 107, 1368
2001
- A Two-Dimensional Alfvén-Wave-Driven Solar Wind Model [42]
Chen, Y. & Hu, Y. Q., Solar Physics, 199, 371
2000
- Solitary kinetic Alfvén waves in the inertial limit region [13]
Chen, Yao, Li, Zhong-yuan, Liu, Wei & Shi, Zhi-Dong, Physics of Plasmas, 7, 371
Created on Wed Apr 22 04:27:27 2026.
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