Publications of Chaowei Jiang

A list of publications authored or co-authored by Chaowei Jiang, 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: 0000-0002-7018-6862

List of publications ordered by citations
Number of papers: 66 (refereed: 65)
No. of citations: 2025
First author papers: 19 (refereed: 19)

2026

  1. Application of a Grid-constrained U-shaped Neural Operator in Real-time Solar Corona Magnetic Field Extrapolation [0]
    Yang, Hao, Zuo, Pingbing, Liu, Zhenhua, Zou, Peng, Jiang, Chaowei, Zou, Zhengyang, Huang, Yanshi, Wang, Yi, Zhang, Kun & Zhang, Ruize, ApJS, 283, 56

2025

  1. The Role of Photospheric Magnetic Flux Diffusion in Initiation of Solar Eruptions [0]
    Bian, Xinkai, Jiang, Chaowei, Wang, Yang, Zou, Peng, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, Solar Physics, 300, 143
  2. A time-dependent three-dimensional dayside magnetopause model based on quasi-elastodynamic theory [1]
    Gu, Yaxin, Wang, Yi, Wei, Fengsi, Feng, Xueshang, Samsonov, Andrey, Song, Xiaojian, Wang, Boyi, Zuo, Pingbing, Jiang, Chaowei, Chen, Yalan, Xu, Xiaojun & Zhou, Zilu, Geoscientific Model Development, 18, 4215
  3. A new method of handling nonlinear discontinuities in a fourth-order conservation element and solution element scheme for magnetohydrodynamic simulations [1]
    Zhang, Ling & Jiang, Chaowei, Physics of Fluids, 37, 106115

2024

  1. Developments of a fundamental mechanism for initiation of solar eruptions [7]
    Jiang, Chaowei, Bian, Xinkai, Feng, Xueshang, Zhou, Zhenjun, Duan, Aiying, Wang, Xinyi, Zou, Peng, Zuo, Pingbing & Wang, Yi, Reviews of Modern Plasma Physics, 8, 18
  2. Assessment of Numerical Weather Models With Different Spatial Resolutions on Tropospheric Delay Correction for InSAR [4]
    Ma, Yongchao, Liu, Tong, Yu, Zhibin, Jiang, Chaowei & Lu, Zhiping, IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, 17, 14133

2023

  1. A Fundamental Mechanism of Solar Eruption Initiation in a Multipolar Magnetic Field [5]
    Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, ApJ, 956, 73
  2. A Study of Preflare Solar Coronal Magnetic Fields: Magnetic Energy and Helicity [8]
    Duan, Aiying, Jiang, Chaowei & Feng, Xueshang, ApJ, 945, 102
  3. Quasi-elastodynamic Processes Involved in the Interaction between Solar Wind and Magnetosphere [2]
    Gu, Y. X., Wang, Y., Wei, F. S., Feng, X. S., Song, X. J., Wang, B. Y., Zuo, P. B., Jiang, C. W., Xu, X. J. & Zhou, Z. L., ApJ, 946, 102
  4. Numerical Simulation of Solar Magnetic Flux Emergence Using the AMR-CESE-MHD Code [3]
    Liu, Zhipeng, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, ApJS, 264, 13
  5. Planar Magnetic Structures Downstream of Coronal Mass Ejection-driven Shocks in the Inner Heliosphere [6]
    Ruan, Mengsi, Zuo, Pingbing, Feng, Xueshang, Xu, Qi, Zhou, Zilu, Wei, Jiayun, Jiang, Chaowei, Wang, Yi, Xu, Xiaojun & Shen, Zhenning, ApJ, 951, 47
  6. MHD Simulation of a Solar Eruption from Active Region 11429 Driven by a Photospheric Velocity Field [9]
    Wang, Xinyi, Jiang, Chaowei & Feng, Xueshang, ApJ, 942, L41
  7. Quantification of the Writhe Number of the Evolution of Solar Filament Axes [2]
    Zhou, Zhenjun, Jiang, Chaowei, Song, Hongqiang, Wang, Yuming, Hao, Yongqiang & Cui, Jun, ApJ, 944, 175

2022

  1. Numerical simulation of a fundamental mechanism of solar eruption with a range of magnetic flux distributions [19]
    Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing, Wang, Yi & Wang, Xinyi, A&A, 658, A174
  2. Homologous Coronal Mass Ejections Caused by Recurring Formation and Disruption of Current Sheet within a Sheared Magnetic Arcade [15]
    Bian, Xinkai, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, ApJ, 925, L7
  3. Quantitative Characterization of Magnetic Flux Rope Properties for Two Solar Eruption Events [14]
    He, Wen, Hu, Qiang, Jiang, Chaowei, Qiu, Jiong & Prasad, Avijeet, ApJ, 934, 103
  4. Data-driven modeling of solar coronal magnetic field evolution and eruptions [53]
    Jiang, Chaowei, Feng, Xueshang, Guo, Yang & Hu, Qiang, The Innovation, 3, 100236
  5. Length Scale of Photospheric Granules in Solar Active Regions [3]
    Liu, Yan-Xiao, Jiang, Chao-Wei, Yuan, Ding, Zuo, Ping-Bing & Cao, Wen-Da, Research in Astronomy and Astrophysics, 22, 085008
  6. Dynamics of the Transversal Magnetic Fields in Photospheric Quiet Regions [1]
    Liu, Yanxiao, Jiang, Chaowei, Yuan, Ding & Zuo, Pingbing, ApJ, 928, 107
  7. Mechanism of the Failed Eruption of an Intermediate Solar Filament [11]
    Peng, Zou, Chaowei, Jiang, Juntao, Wang & Xinkai, Bian, ApJ, 928, 160
  8. MHD Simulation of Homologous Eruptions from Solar Active Region 10930 Caused by Sunspot Rotation [10]
    Wang, Xinyi, Jiang, Chaowei, Feng, Xueshang, Duan, Aiying & Bian, Xinkai, ApJ, 938, 61
  9. Fast plasmoid-mediated reconnection in a solar flare [72]
    Yan, Xiaoli, Xue, Zhike, Jiang, Chaowei, Priest, E. R., Kliem, Bernhard, Yang, Liheng, Wang, Jincheng, Kong, Defang, Song, Yongliang, Feng, Xueshang & Liu, Zhong, Nature Communications, 13, 640
  10. The Rotation of Magnetic Flux Ropes Formed during Solar Eruption [18]
    Zhou, Zhenjun, Jiang, Chaowei, Liu, Rui, Wang, Yuming, Liu, Lijuan & Cui, Jun, ApJ, 927, L14

2021

  1. Variation of Magnetic Flux Ropes through Major Solar Flares [8]
    Duan, Aiying, Jiang, Chaowei, Zhou, Zhenjun, Feng, Xueshang & Cui, Jun, ApJ, 907, L23
  2. Structure and Evolution of an Inter-Active Region Large-scale Magnetic Flux Rope [8]
    Duan, Aiying, Jiang, Chaowei, Zou, Peng, Feng, Xueshang & Cui, Jun, ApJ, 906, 45
  3. A fundamental mechanism of solar eruption initiation [144]
    Jiang, Chaowei, Feng, Xueshang, Liu, Rui, Yan, XiaoLi, Hu, Qiang, Moore, Ronald L., Duan, Aiying, Cui, Jun, Zuo, Pingbing, Wang, Yi & Wei, Fengsi, Nature Astronomy, 5, 1126
  4. Investigations of Sizes and Dynamical Motions of Solar Photospheric Granules by a Novel Granular Segmenting Algorithm [7]
    Liu, Yanxiao, Jiang, Chaowei, Yuan, Ding, Zuo, Pingbing, Wang, Yi & Cao, Wenda, ApJ, 923, 133
  5. Diagnosing a Solar Flaring Core with Bidirectional Quasi-periodic Fast Propagating Magnetoacoustic Waves [21]
    Miao, Yuhu, Li, Dong, Yuan, Ding, Jiang, Chaowei, Elmhamdi, Abouazza, Zhao, Mingyu & Anfinogentov, Sergey, ApJ, 908, L37
  6. The Causes of Peripheral Coronal Loop Contraction and Disappearance Revealed in a Magnetohydrodynamic Simulation of Solar Eruption [8]
    Wang, Juntao, Jiang, Chaowei, Yuan, Ding & Zou, Peng, ApJ, 911, 2
  7. Evidence of wave-wave coupling between frequency harmonic bands of magnetosonic waves [5]
    Zou, Zhengyang, Gao, Zhonglei, Zuo, Pingbing, Ni, Binbin, Wang, Geng, Zhao, Zhengyu, Feng, Xueshang, Xu, Xiaojun, Jiang, Chaowei, Wang, Yi & Wei, Fengsi, Physics of Plasmas, 28, 122903

2020

  1. On the Lorentz Force and Torque of Solar Photospheric Emerging Magnetic Fields [6]
    Duan, Aiying, Jiang, Chaowei, Toriumi, Shin & Syntelis, Petros, ApJ, 896, L9
  2. Data-driven MHD Simulation of the Formation and Initiation of a Large-scale Preflare Magnetic Flux Rope in AR 12371 [20]
    He, Wen, Jiang, Chaowei, Zou, Peng, Duan, Aiying, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, ApJ, 892, 9
  3. Testing a Data-driven Active Region Evolution Model with Boundary Data at Different Heights from a Solar Magnetic Flux Emergence Simulation [10]
    Jiang, Chaowei & Toriumi, Shin, ApJ, 903, 11
  4. Two Quasi-periodic Fast-propagating Magnetosonic Wave Events Observed in Active Region NOAA 11167 [18]
    Miao, Yuhu, Liu, Yu, Elmhamdi, A., Kordi, A. S., Shen, Y. D., Al-Shammari, Rehab, Al-Mosabeh, Khaled, Jiang, Chaowei & Yuan, Ding, ApJ, 889, 139
  5. Comparative Study of Data-driven Solar Coronal Field Models Using a Flux Emergence Simulation as a Ground-truth Data Set [34]
    Toriumi, Shin, Takasao, Shinsuke, Cheung, Mark C. M., Jiang, Chaowei, Guo, Yang, Hayashi, Keiji & Inoue, Satoshi, ApJ, 890, 103
  6. The Relationship between Chirality, Sense of Rotation, and Hemispheric Preference of Solar Eruptive Filaments [19]
    Zhou, Zhenjun, Liu, Rui, Cheng, Xing, Jiang, Chaowei, Wang, Yuming, Liu, Lijuan & Cui, Jun, ApJ, 891, 180
  7. Continuous Null-point Magnetic Reconnection Builds Up a Torus Unstable Magnetic Flux Rope Triggering the X9.3 Flare in Solar AR 12673 [25]
    Zou, Peng, Jiang, Chaowei, Wei, Fengsi, Feng, Xueshang, Zuo, Pingbing & Wang, Yi, ApJ, 890, 10

2019

  1. A Study of Pre-flare Solar Coronal Magnetic Fields: Magnetic Flux Ropes [67]
    Duan, Aiying, Jiang, Chaowei, He, Wen, Feng, Xueshang, Zou, Peng & Cui, Jun, ApJ, 884, 73
  2. Magnetohydrodynamic Simulations for Solar Active Regions using Time-series Data of Surface Plasma Flow and Electric Field Inferred from Helioseismic Magnetic Imager Vector Magnetic Field Measurements [29]
    Hayashi, Keiji, Feng, Xueshang, Xiong, Ming & Jiang, Chaowei, ApJ, 871, L28
  3. Intermittent Heating in the Magnetic Cloud Sheath Regions [3]
    Zhou, Zilu, Zuo, Pingbing, Wei, Fengsi, Feng, Xueshang, Wang, Yi, Wang, Ludi, Jiang, Chaowei, Song, Xiaojian & Xu, Xiaojun, ApJ, 885, L13
  4. A Statistical Study of Solar Filament Eruptions that Form High-speed Coronal Mass Ejections [33]
    Zou, Peng, Jiang, Chaowei, Wei, Fengsi, Zuo, Pingbing & Wang, Yi, ApJ, 884, 157
  5. A Two-step Magnetic Reconnection in a Confined X-class Flare in Solar Active Region 12673 [35]
    Zou, Peng, Jiang, Chaowei, Feng, Xueshang, Zuo, Pingbing, Wang, Yi & Wei, Fengsi, ApJ, 870, 97

2018

  1. An MHD Simulation of Solar Active Region 11158 Driven with a Time-dependent Electric Field Determined from HMI Vector Magnetic Field Measurement Data [56]
    Hayashi, Keiji, Feng, Xueshang, Xiong, Ming & Jiang, Chaowei, ApJ, 855, 11
  2. Magnetohydrodynamic Simulation of the X9.3 Flare on 2017 September 6: Evolving Magnetic Topology [61]
    Jiang, Chaowei, Zou, Peng, Feng, Xueshang, Hu, Qiang, Liu, Rui, Vemareddy, P., Duan, Aiying, Zuo, Pingbing, Wang, Yi & Wei, Fengsi, ApJ, 869, 13
  3. Formation and Eruption of an Active Region Sigmoid. II. Magnetohydrodynamic Simulation of a Multistage Eruption [30]
    Jiang, Chaowei, Feng, Xueshang & Hu, Qiang, ApJ, 866, 96

2017

  1. Comparison of Two Coronal Magnetic Field Models to Reconstruct a Sigmoidal Solar Active Region with Coronal Loops [23]
    Duan, Aiying, Jiang, Chaowei, Hu, Qiang, Zhang, Huai, Gary, G. Allen, Wu, S. T. & Cao, Jinbin, ApJ, 842, 119
  2. Reconstruction of a Large-scale Pre-flare Coronal Current Sheet Associated with a Homologous X-shaped Flare [16]
    Jiang, Chaowei, Yan, Xiaoli, Feng, Xueshang, Duan, Aiying, Hu, Qiang, Zuo, Pingbing & Wang, Yi, ApJ, 850, 8
  3. Observation of a Large-scale Quasi-circular Secondary Ribbon Associated with Successive Flares and a Halo CME [8]
    Lim, Eun-Kyung, Yurchyshyn, Vasyl, Kumar, Pankaj, Cho, Kyuhyoun, Jiang, Chaowei, Kim, Sujin, Yang, Heesu, Chae, Jongchul, Cho, Kyung-Suk & Lee, Jeongwoo, ApJ, 850, 167
  4. Buildup of a highly twisted magnetic flux rope during a solar eruption [93]
    Wang, Wensi, Liu, Rui, Wang, Yuming, Hu, Qiang, Shen, Chenglong, Jiang, Chaowei & Zhu, Chunming, Nature Communications, 8, 1330
  5. The Eruption of a Small-scale Emerging Flux Rope as the Driver of an M-class Flare and of a Coronal Mass Ejection [36]
    Yan, X. L., Jiang, C. W., Xue, Z. K., Wang, J. C., Priest, E. R., Yang, L. H., Kong, D. F., Cao, W. D. & Ji, H. S., ApJ, 845, 18

2016

  1. How Did a Major Confined Flare Occur in Super Solar Active Region 12192? [89]
    Jiang, Chaowei, Wu, S. T., Yurchyshyn, Vasyl, Wang, Haiming, Feng, Xueshang & Hu, Qiang, ApJ, 828, 62

2014

  1. Preprocessing the Photospheric Vector Magnetograms for an NLFFF Extrapolation Using a Potential-Field Model and an Optimization Method [36]
    Jiang, Chaowei & Feng, Xueshang, Solar Physics, 289, 63
  2. Nonlinear Force-free Field Extrapolation of a Coronal Magnetic Flux Rope Supporting a Large-scale Solar Filament from a Photospheric Vector Magnetogram [68]
    Jiang, Chaowei, Wu, S. T., Feng, Xueshang & Hu, Qiang, ApJ, 786, L16
  3. Formation and Eruption of an Active Region Sigmoid. I. A Study by Nonlinear Force-free Field Modeling [95]
    Jiang, Chaowei, Wu, S. T., Feng, Xueshang & Hu, Qiang, ApJ, 780, 55
  4. Simulation of sigmoid structure and filament eruption of AR11283 using a three-dimensional data-driven magnetohydrodynamic model [1]
    Wu, S. T., Jiang, Chaowei, Feng, Xueshang, Hu, Qiang & Liu, Yang, Nature of Prominences and their Role in Space Weather (Editors: Schmieder, Brigitte, Malherbe, Jean-Marie & Wu, S. T.), IAU Symposium, 300, p. 466

2013

  1. Magnetohydrodynamic Simulation of a Sigmoid Eruption of Active Region 11283 [134]
    Jiang, Chaowei, Feng, Xueshang, Wu, S. T. & Hu, Qiang, ApJ, 771, L30
  2. Extrapolation of the Solar Coronal Magnetic Field from SDO/HMI Magnetogram by a CESE-MHD-NLFFF Code [80]
    Jiang, Chaowei & Feng, Xueshang, ApJ, 769, 144
  3. Magnetic Reconnection: From "Open" Extreme-ultraviolet Loops to Closed Post-flare Ones Observed by SDO [15]
    Zhang, Jun, Yang, Shuhong, Li, Ting, Zhang, Yuzong, Li, Leping & Jiang, Chaowei, ApJ, 776, 57

2012

  1. A Data-driven Model for the Global Coronal Evolution [77]
    Feng, Xueshang, Jiang, Chaowei, Xiang, Changqing, Zhao, Xuepu & Wu, S. T., ApJ, 758, 62
  2. A Unified and Very Fast Way for Computing the Global Potential and Linear Force-Free Fields [18]
    Jiang, Chaowei & Feng, Xueshang, Solar Physics, 281, 621
  3. 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 [37]
    Jiang, Chaowei, Feng, Xueshang, Wu, S. T. & Hu, Qiang, ApJ, 759, 85
  4. A New Code for Nonlinear Force-free Field Extrapolation of the Global Corona [31]
    Jiang, Chaowei, Feng, Xueshang & Xiang, Changqing, ApJ, 755, 62
  5. A New Implementation of the Magnetohydrodynamics-relaxation Method for Nonlinear Force-free Field Extrapolation in the Solar Corona [54]
    Jiang, Chaowei & Feng, Xueshang, ApJ, 749, 135

2011

  1. A Hybrid Solar Wind Model of the CESE+HLL Method with a Yin-Yang Overset Grid and an AMR Grid [73]
    Feng, Xueshang, Zhang, Shaohua, Xiang, Changqing, Yang, Liping, Jiang, Chaowei & Wu, S. T., ApJ, 734, 50
  2. Reconstruction of the Coronal Magnetic Field Using the CESE-MHD Method [44]
    Jiang, Chaowei, Feng, Xueshang, Fan, Yuliang & Xiang, Changqing, ApJ, 727, 101

2010

  1. AMR Simulations of Magnetohydrodynamic Problems by the CESE Method in Curvilinear Coordinates [86]
    Jiang, Chaowei, Feng, Xueshang, Zhang, Jian & Zhong, Dingkun, Solar Physics, 267, 463

Created on Wed Apr 22 04:25:56 2026.