Flux Rope Model of the 2003 October 28–30 Coronal Mass Ejection and Interplanetary Coronal Mass Ejection

2006 ◽  
Vol 642 (1) ◽  
pp. 541-553 ◽  
Author(s):  
J. Krall ◽  
V. B. Yurchyshyn ◽  
S. Slinker ◽  
R. M. Skoug ◽  
J. Chen
2016 ◽  
Vol 12 (S327) ◽  
pp. 67-70
Author(s):  
J. Palacios ◽  
C. Cid ◽  
E. Saiz ◽  
A. Guerrero

AbstractWe have investigated the case of a coronal mass ejection that was eroded by the fast wind of a coronal hole in the interplanetary medium. When a solar ejection takes place close to a coronal hole, the flux rope magnetic topology of the coronal mass ejection (CME) may become misshapen at 1 AU as a result of the interaction. Detailed analysis of this event reveals erosion of the interplanetary coronal mass ejection (ICME) magnetic field. In this communication, we study the photospheric magnetic roots of the coronal hole and the coronal mass ejection area with HMI/SDO magnetograms to define their magnetic characteristics.


1999 ◽  
Author(s):  
T. Mulligan ◽  
C. T. Russell ◽  
B. J. Anderson ◽  
D. A. Lohr ◽  
B. A. Toth ◽  
...  

2010 ◽  
Vol 725 (1) ◽  
pp. L84-L90 ◽  
Author(s):  
Rui Liu ◽  
Chang Liu ◽  
Shuo Wang ◽  
Na Deng ◽  
Haimin Wang

Author(s):  
N. U. Crooker ◽  
J. T. Gosling ◽  
E. J. Smith ◽  
C. T. Russell

1997 ◽  
Vol 490 (2) ◽  
pp. L191-L194 ◽  
Author(s):  
J. Chen ◽  
R. A. Howard ◽  
G. E. Brueckner ◽  
R. Santoro ◽  
J. Krall ◽  
...  

1999 ◽  
Vol 26 (16) ◽  
pp. 2613-2616 ◽  
Author(s):  
W. C. Feldman ◽  
R. M. Skoug ◽  
J. T. Gosling ◽  
D. J. McComas ◽  
R. L. Tokar ◽  
...  

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