Asymmetric variations of the coronal green line intensity

Solar Physics ◽  
1988 ◽  
Vol 115 (2) ◽  
pp. 367-384 ◽  
Author(s):  
V. P. Tritakis ◽  
H. Mavromichalaki ◽  
B. Petropoulos
Solar Physics ◽  
1975 ◽  
Vol 41 (2) ◽  
pp. 349-366 ◽  
Author(s):  
E. C. Roelof ◽  
S. Cuperman ◽  
A. Sternlieb

2000 ◽  
Vol 179 ◽  
pp. 197-200
Author(s):  
Milan Minarovjech ◽  
Milan Rybanský ◽  
Vojtech Rušin

AbstractWe present an analysis of short time-scale intensity variations in the coronal green line as obtained with high time resolution observations. The observed data can be divided into two groups. The first one shows periodic intensity variations with a period of 5 min. the second one does not show any significant intensity variations. We studied the relation between regions of coronal intensity oscillations and the shape of white-light coronal structures. We found that the coronal green-line oscillations occur mainly in regions where open white-light coronal structures are located.


2005 ◽  
Vol 49 (6) ◽  
pp. 477-484 ◽  
Author(s):  
O. G. Badalyan ◽  
V. N. Obridko ◽  
J. Sýkora

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