OBSERVATIONS AND MAGNETIC FIELD MODELING OF THE FLARE/CORONAL MASS EJECTION EVENT ON 2010 APRIL 8

2011 ◽  
Vol 734 (1) ◽  
pp. 53 ◽  
Author(s):  
Yingna Su ◽  
Vincent Surges ◽  
Adriaan van Ballegooijen ◽  
Edward DeLuca ◽  
Leon Golub
2018 ◽  
Vol 868 (1) ◽  
pp. 59 ◽  
Author(s):  
Tie Liu ◽  
Yingna Su ◽  
Xin Cheng ◽  
Adriaan van Ballegooijen ◽  
Haisheng Ji

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.


1992 ◽  
Vol 97 (A2) ◽  
pp. 1597 ◽  
Author(s):  
L. C. Tan ◽  
G. M. Mason ◽  
M. A. Lee ◽  
B. Klecker ◽  
F. M. Ipavich

Sign in / Sign up

Export Citation Format

Share Document