24 citations as recorded by crossref.

1. The Solar Wind Speed Expansion Factor [${v}$–$f _{\text{s}}$] Relationship at the Inner Boundary (18 $\text{R}_{\odot }$) of the Heliosphere C. Wu et al. 10.1007/s11207-019-1576-6
2. A 2.5‐dimensional MHD parametric study of interplanetary shock interactions with the heliospheric current sheet/heliospheric plasma sheet Z. Smith et al. 10.1029/98JA01994
3. Determining the parameters of coronal mass ejections using the method of MHD modeling ejection evolutions N. Barkhatov et al. 10.1134/S0016793210030047
4. A Novel Numerical Implementation for Solar Wind Modeling by the Modified Conservation Element/Solution Element Method X. Feng et al. 10.1086/510121
5. Three‐dimensional MHD simulation of CMEs in three‐dimensional background solar wind with the self‐consistent structure on the source surface as input: Numerical simulation of the January 1997 Sun‐Earth connection event F. Shen et al. 10.1029/2006JA012164
6. Three-dimensional global simulation of multiple ICMEs’ interaction and propagation from the Sun to the heliosphere following the 25–28 October 2003 solar events C. Wu et al. 10.1016/j.asr.2007.06.025
7. A large polar crown coronal mass ejection and a “problem” goemagnetic storm: April 14–23, 1994 A. McAllister et al. 10.1029/96JA00510
8. Numerical simulation of the 12 May 1997 interplanetary CME event D. Odstrcil et al. 10.1029/2003JA010135
9. COUPLING OF CORONAL AND HELIOSPHERIC MAGNETOHYDRODYNAMIC MODELS: SOLUTION COMPARISONS AND VERIFICATION V. Merkin et al. 10.3847/0004-637X/831/1/23
10. Predicting the Arrival Time of Shock Passages at Earth C. Wu et al. 10.1007/s11207-005-1213-4
11. Reply [to “Comment on “The solar energetic particle event of April 14, 1994, as a probe of shock formation and particle acceleration” by S. W. Kahler, H. V. Cane, H. S. Hudson, V. G. Kurt, Y. V. Gotselyuk, R. J. MacDowall, and V. Bothmer”] S. Kahler et al. 10.1029/1999JA900235
12. Flare‐generated shock evolution and geomagnetic storms during the “Halloween 2003 epoch”: 29 October to 2 November C. Wu et al. 10.1029/2005JA011011
13. Forecast evaluation of the coronal mass ejection (CME) geoeffectiveness using halo CMEs from 1997 to 2003 R. Kim et al. 10.1029/2005JA011218
14. On the overtaking interaction of typical shock waves in the solar wind flow S. Grib 10.1134/S1063773710010068
15. Models of Solar Wind Structures and Their Interaction with the Earth’s Space Environment J. Watermann et al. 10.1007/s11214-009-9494-9
16. Global simulation of extremely fast coronal mass ejection on 23 July 2012 K. Liou et al. 10.1016/j.jastp.2014.09.013
17. Distortion of the interplanetary magnetic field by three‐dimensional propagation of coronal mass ejections in a structured solar wind D. Odstrcil & V. Pizzo 10.1029/1999JA900319
18. Recipe for predicting the IMF Bz polarity's change of direction following solar disturbances and at the onset of geomagnetic storms C. Wu et al. 10.1016/0021-9169(96)00010-4
19. Three‐dimensional global simulation of interplanetary coronal mass ejection propagation from the Sun to the heliosphere: Solar event of 12 May 1997 C. Wu et al. 10.1029/2006JA012211
20. Validation of a global 3D heliospheric model with observations for the May 12, 1997 CME event O. Cohen et al. 10.1016/j.jastp.2007.08.065
21. predicting the initial IMF Bz polarity's change at 1 AU caused by shocks that precede coronal mass ejections C. Wu & M. Dryer 10.1029/96GL01721
22. Generation and propagation of solar disturbances: a magnetohydrodynamic simulation S. Wu & W. Guo 10.1016/S1364-6826(98)00121-7
23. Three‐dimensional MHD simulation of the April 14, 1994, interplanetary coronal mass ejection and its propagation to Earth and Ulysses M. Dryer et al. 10.1029/97JA00872
24. Modeling inner boundary values at 18 solar radii during solar quiet time for global three-dimensional time-dependent magnetohydrodynamic numerical simulation C. Wu et al. 10.1016/j.jastp.2020.105211