MHD waves in the solar north polar coronal hole

2010 ◽  
Vol 331 (7) ◽  
pp. 716-724 ◽  
Author(s):  
E. Devlen ◽  
E.R. Pekünlü
2017 ◽  
Vol 467 (1) ◽  
pp. 133-144
Author(s):  
E. Devlen ◽  
D. Zengin Çamurdan ◽  
M. Yardımcı ◽  
E. R. Pekünlü

2010 ◽  
Vol 6 (S274) ◽  
pp. 137-139
Author(s):  
Suzan Doğan ◽  
E. Rennan Pekünlü

AbstractThe effect of the Plume/Interplume Lane (PIPL) structure of the solar North Polar Coronal Hole (NPCH) on the ion-cyclotron resonance (ICR) process is investigated. The ICR process in the interplume lanes is much more effective than in the plumes, agreeing with the observations which show the source of fast solar wind is interplume lanes.


2002 ◽  
Vol 30 (3) ◽  
pp. 523-528
Author(s):  
L. Zangrilli ◽  
G. Poletto ◽  
P. Nicolosi ◽  
G. Noci

1997 ◽  
Vol 490 (2) ◽  
pp. L187-L190 ◽  
Author(s):  
H. P. Warren ◽  
J. T. Mariska ◽  
K. Wilhelm

Solar Physics ◽  
1977 ◽  
Vol 51 (2) ◽  
pp. 399-407 ◽  
Author(s):  
Serge Koutchmy

2010 ◽  
Author(s):  
E. C. Roelof ◽  
R. B. Decker ◽  
S. M. Krimigis ◽  
M. Maksimovic ◽  
K. Issautier ◽  
...  

Author(s):  
S. Patsourakos ◽  
J.-C. Vial ◽  
J.-R. Gabryl ◽  
S. Koutchmy ◽  
U. Schühle

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