| Data-driven magnetohydrodynamic modelling of a flux-emerging active region leading to solar eruption C Jiang, ST Wu, X Feng, Q Hu Nature communications 7 (1), 11522, 2016 | 148 | 2016 |
| Formation and eruption of an active region sigmoid. I. A study by nonlinear force-free field modeling C Jiang, ST Wu, X Feng, Q Hu The Astrophysical Journal 780 (1), 55, 2013 | 102 | 2013 |
| Magnetohydrodynamic simulation of a sigmoid eruption of active region 11283 C Jiang, X Feng, ST Wu, Q Hu The Astrophysical Journal Letters 771 (2), L30, 2013 | 100 | 2013 |
| AMR simulations of magnetohydrodynamic problems by the CESE method in curvilinear coordinates C Jiang, X Feng, J Zhang, D Zhong Solar Physics 267, 463-491, 2010 | 96 | 2010 |
| A hybrid solar wind model of the cese+ hll method with a Yin–Yang overset grid and an AMR grid X Feng, S Zhang, C Xiang, L Yang, C Jiang, ST Wu The Astrophysical Journal 734 (1), 50, 2011 | 93 | 2011 |
| A data-driven model for the global coronal evolution X Feng, C Jiang, C Xiang, X Zhao, ST Wu The Astrophysical Journal 758 (1), 62, 2012 | 90 | 2012 |
| How did a major confined flare occur in super solar active region 12192? C Jiang, ST Wu, V Yurchyshyn, H Wang, X Feng, Q Hu The Astrophysical Journal 828 (1), 62, 2016 | 87 | 2016 |
| A fundamental mechanism of solar eruption initiation C Jiang, X Feng, R Liu, XL Yan, Q Hu, RL Moore, A Duan, J Cui, P Zuo, ... Nature Astronomy 5 (11), 1126-1138, 2021 | 82 | 2021 |
| Extrapolation of the solar coronal magnetic field from sdo/hmi magnetogram by a cese–mhd–nlfff code C Jiang, X Feng The Astrophysical Journal 769 (2), 144, 2013 | 79 | 2013 |
| 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 | 67 | 2017 |
| A new implementation of the magnetohydrodynamics-relaxation method for nonlinear force-free field extrapolation in the solar corona C Jiang, X Feng The Astrophysical Journal 749 (2), 135, 2012 | 66 | 2012 |
| A study of pre-flare solar coronal magnetic fields: magnetic flux ropes A Duan, C Jiang, W He, X Feng, P Zou, J Cui The Astrophysical Journal 884 (1), 73, 2019 | 57 | 2019 |
| Magnetohydrodynamic simulation of the X9. 3 flare on 2017 September 6: evolving magnetic topology C Jiang, P Zou, X Feng, Q Hu, R Liu, P Vemareddy, A Duan, P Zuo, ... The Astrophysical Journal 869 (1), 13, 2018 | 54 | 2018 |
| Three-dimensional magnetic restructuring in two homologous solar flares in the seismically active NOAA AR 11283 C Liu, N Deng, J Lee, T Wiegelmann, C Jiang, BR Dennis, Y Su, A Donea, ... The Astrophysical Journal 795 (2), 128, 2014 | 47 | 2014 |
| An MHD simulation of solar active region 11158 driven with a time-dependent electric field determined from HMI vector magnetic field measurement data K Hayashi, X Feng, M Xiong, C Jiang The Astrophysical Journal 855 (1), 11, 2018 | 45 | 2018 |
| Nonlinear force-free field extrapolation of a coronal magnetic flux rope supporting a large-scale solar filament from a photospheric vector magnetogram C Jiang, ST Wu, X Feng, Q Hu The Astrophysical Journal Letters 786 (2), L16, 2014 | 45 | 2014 |
| RECONSTRUCTION OF THE CORONAL MAGNETIC FIELD USING THE CESE–MHD METHOD C Jiang, X Feng, Y Fan, C Xiang The Astrophysical Journal 727 (2), 101, 2011 | 43 | 2011 |
| Preprocessing the photospheric vector magnetograms for an NLFFF extrapolation using a potential-field model and an optimization method C Jiang, X Feng Solar Physics 289, 63-77, 2014 | 41 | 2014 |
| 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 C Jiang, X Feng, ST Wu, Q Hu The Astrophysical Journal 759 (2), 85, 2012 | 40 | 2012 |
| Fast plasmoid-mediated reconnection in a solar flare X Yan, Z Xue, C Jiang, ER Priest, B Kliem, L Yang, J Wang, D Kong, ... Nature Communications 13 (1), 640, 2022 | 36 | 2022 |
Qiang HuProfessor of Space Science, University of Alabama in HuntsvilleEmail verificata su uah.edu
