236 citations · 352 across the 6 of their papers we have counts for
6 papers
Modeling Inner Boundary Values at 18 Solar Radii During Solar Quiet time for Global Three-dimensional Time-Dependent Magnetohydrodynamic Numerical Simulation
Chin-Chun Wu, Kan Liou, Simon Plunkett +6
The solar wind speed plays a key role in the transport of CME out of the Sun and ultimately determines the arrival time of CME-driven shocks in the heliosphere. Here, we develop an…
Comparison of Two Coronal Magnetic Field Models for Reconstructing a Sigmoidal Solar Active Region With Coronal Loops
Aiying Duan, Chaowei Jiang, Qiang Hu +4
Magnetic field extrapolation is an important tool to study the three-dimensional (3D) solar coronal magnetic field which is difficult to directly measure. Various analytic models a…
Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness: 2. Oblique collision
Ming Xiong, Huinan Zheng, Shui Wang
The numerical studies of the interplanetary coupling between multiple magnetic clouds (MCs) are continued by a 2.5-dimensional ideal magnetohydrodynamic (MHD) model in the heliosph…
Magnetohydrodynamic simulation of the interaction between two interplanetary magnetic clouds and its consequent geoeffectiveness
Ming Xiong, Huinan Zheng, S. T. Wu +2
Numerical studies of the interplanetary "multiple magnetic clouds (Multi-MC)" are performed by a 2.5-dimensional ideal magnetohydrodynamic (MHD) model in the heliospheric meridiona…
Magnetic topologies and two-class coronal mass ejections: a numerical magnetohydrodynamic study
W. Liu, X. P. Zhao, S. T. Wu +1
White-light observations of the solar corona show that there are two characteristic types of Coronal Mass Ejections (CMEs) in terms of speed-height profiles: so-called fast CMEs th…
Direct Detection of a CME-Associated Shock in LASCO White Light Images
A. Vourlidas, S. T. Wu, A. H. Wang +2
The LASCO C2 and C3 coronagraphs recorded a unique coronal mass ejection on April 2, 1999. The event did not have the typical three-part CME structure and involved a small filament…