|
Feng, X. |
Volume |
Paper Title |
Page Number |
Authors |
459 |
Numerical Study of the Global Corona for CR 2055 Driven by Daily Updated Synoptic Magnetic Field |
202 |
Feng, X.; Yang, L. P.; Xiang, C. Q.; Liu, Y.; Zhao, X.; Wu, S. T. |
459 |
3D MHD Numerical Study of Two CMEs' Evolution and Their Interaction |
247 |
Shen, F.; Feng, X.; Wu, S. T. |
459 |
Modeling of Solar Active Region Using a Three-Dimensional, Time-Dependent, Data-Driven Magnetohydrodynamic Model |
254 |
Wu, S. T.; Wang, A. H.; Falconer, D.; Hu, Q.; Liu, Y.; Feng, X.; Shen, F. |
474 |
GPU Computing in Space Weather Modeling |
131 |
Feng, X.; Zhong, D.; Xiang, C.; Zhang, Y. |
474 |
Modeling Source Surface Plasma and Magnetic Field Based on Expansion Factor fS and Angular Distance θb Between the Foot Points |
172 |
Shen, F.; Feng, X.; Xiang, C.; Wu, S. T. |
488 |
Energy Analysis During the Collision of Two Successive CMEs |
179 |
Shen, F.; Shen, C.; Wang, Y.; Feng, X.; Xiang, C. |
488 |
Dual Time Stepping Method For three-dimensional MHD With Splitting Based Scheme |
223 |
Feng, X.; Fu, H. |
498 |
Modeling the Global Distribution of Plasma Parameters on Coronal Source Surface for Different Solar Phases Using 1AU Observations |
168 |
Yang, Y.; Shen, F.; Feng, X. |
|
|