Three-dimensional propagation of coronal mass ejections (CMEs) in a structured solar wind flow: 1. CME launched within the streamer belt

1999 ◽  
Vol 104 (A1) ◽  
pp. 483-492 ◽  
Author(s):  
D. Odstrčil ◽  
V. J. Pizzo
2011 ◽  
Vol 743 (2) ◽  
pp. 101 ◽  
Author(s):  
Manuela Temmer ◽  
Tanja Rollett ◽  
Christian Möstl ◽  
Astrid M. Veronig ◽  
Bojan Vršnak ◽  
...  

2007 ◽  
Vol 73 (2) ◽  
pp. 145-151 ◽  
Author(s):  
LARS G. WESTERBERG ◽  
H.O. ÅKERSTEDT

Abstract.An improvement of an existing three-dimensional analytical model describing the solar wind flow near a reconnection site at the dayside magnetopause is reported. Introducing an arbitrary orientation of the reconnection line, general solutions for the plasma velocity and magnetic field during the transition of the magnetopause are presented, together with the development of the magnetopause transition layer away from the reconnection site.


2007 ◽  
Vol 55 (12) ◽  
pp. 1793-1803 ◽  
Author(s):  
H.K. Biernat ◽  
N.V. Erkaev ◽  
U.V. Amerstorfer ◽  
T. Penz ◽  
H.I.M. Lichtenegger

1996 ◽  
Vol 101 (A5) ◽  
pp. 10665-10672 ◽  
Author(s):  
N. V. Erkaev ◽  
C. J. Farrugia ◽  
H. K. Biernat
Keyword(s):  

2000 ◽  
Vol 62 (5) ◽  
pp. 6496-6504 ◽  
Author(s):  
Wiesław M. Macek ◽  
Stefano Redaelli
Keyword(s):  

2003 ◽  
pp. 153-171 ◽  
Author(s):  
M. Neugebauer ◽  
J. T. Steinberg ◽  
R. L. Tokar ◽  
B. L. Barraclough ◽  
E. E. Dors ◽  
...  

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