scholarly journals THE VERY UNUSUAL INTERPLANETARY CORONAL MASS EJECTION OF 2012 JULY 23: A BLAST WAVE MEDIATED BY SOLAR ENERGETIC PARTICLES

2013 ◽  
Vol 770 (1) ◽  
pp. 38 ◽  
Author(s):  
C. T. Russell ◽  
R. A. Mewaldt ◽  
J. G. Luhmann ◽  
G. M. Mason ◽  
T. T. von Rosenvinge ◽  
...  
Solar Physics ◽  
2016 ◽  
Vol 291 (2) ◽  
pp. 487-511 ◽  
Author(s):  
Silja Pohjolainen ◽  
Firas Al-Hamadani ◽  
Eino Valtonen

2020 ◽  
Vol 246 (2) ◽  
pp. 29 ◽  
Author(s):  
J. Giacalone ◽  
D. G. Mitchell ◽  
R. C. Allen ◽  
M. E. Hill ◽  
R. L. McNutt ◽  
...  

2002 ◽  
Vol 64 (5-6) ◽  
pp. 517-525 ◽  
Author(s):  
O.E. Malandraki ◽  
E.T. Sarris ◽  
L.J. Lanzerotti ◽  
P. Trochoutsos ◽  
G. Tsiropoula ◽  
...  

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.


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