Three-dimensional MHD simulation of the evolution of the April 2000 CME event and its induced shocks using a magnetized plasma blob model

A three‐dimensional (3‐D) time‐dependent, numerical magnetohydrodynamic (MHD) model with asynchronous and parallel time‐marching method is used to investigate the propagation of coronal mass ejections (CMEs) in the nonhomogenous background solar wind flow. The background solar wind is constructed ba...

Ausführliche Beschreibung

Bibliographische Detailangaben

Veröffentlicht in:	Journal of Geophysical Research: Space Physics 2011-04, Vol.116 (A4), p.n/a
Hauptverfasser:	Shen, F., Feng, X. S., Wu, S. T., Xiang, C. Q., Song, W. B.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Boundary conditions Earth orbits High temperature Magnetic fields MHD simulation Planetology shock Space Spacecraft
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!