| |
Wu, S. T. |
| Volume |
Paper Title |
Page Number |
Authors |
| 46 |
Magnetohydrodynamics Simulation of the Evolution of Bipolar Magnetic Regions (Invited) |
98 |
Wu, S. T.; Yin, C. L.; McIntosh, P.; Hildner, E. |
| 95 |
Quasi- Three-Dimensional Magnetohydrodynamic Model of the Photospheric Dynamo and Force-Free Model of the Corona for Flare and CME Probability Predictions |
74 |
Fry, C. D.; Wu, S. T.; Yin, C. L. |
| 95 |
Initiation of Solar Disturbances Due to Emerging Magnetic Flux (EMF) |
128 |
Wu, S. T.; Guo, W. P. |
| 429 |
Characteristic Boundary Conditions for Numerical Magnetohydrodynamic (MHD) Simulation of Solar and Laboratory Plasma Flows |
294 |
Wu, S. T.; Wang, A. H.; Cassibry, J. |
| 444 |
A Global Solar Wind Model Based on Surface Measurements of Magnetic Field and
Transverse Velocity from GONG |
143 |
Wu, S. T.; Wang, A. H.; Wu, C.-C.; Hill, F.; Hernández, I. G.; Feng, X. S.; Dryer, M. |
| 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 |
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. |
| 474 |
Evidence of the Correspondence of EIT Waves and Coronal Mass Ejections
Induced Waves Using a Three-Dimensional Magnetohydrodynamic Simulation |
185 |
Wu, S. T.; Wu, C.-C.; Liou, K. |
| 484 |
Analyses of the Evolution and Interaction of Multiple Coronal Mass Ejections and Their Shocks in July 2012 |
241 |
Wu, S. T.; Wu, C.; Liou, K.; Plunkett, S.; Dryer, M.; Fry, C. D. |
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