Twist and Writhe of the Magnetic Flux in the Super Active Region NOAA 11429

2014 ◽  
pp. 335-348 ◽  
Author(s):  
A. Elmhamdi ◽  
P. Romano ◽  
A. S. Kordi ◽  
H. A. Al-trabulsy
1998 ◽  
Vol 167 ◽  
pp. 74-77
Author(s):  
G.A. Porfir’eva ◽  
G.V. Yakunina ◽  
Z. Mouradian

AbstractThe behaviour of extended filaments in the vicinity of a new emerging magnetic flux site has been investigated during the 2N/M5.8 flare on September 1 and several flares on September 2, 1989.


Solar Physics ◽  
2014 ◽  
Vol 289 (8) ◽  
pp. 2957-2970 ◽  
Author(s):  
A. Elmhamdi ◽  
P. Romano ◽  
A. S. Kordi ◽  
H. A. Al-trabulsy

2012 ◽  
Vol 8 (S294) ◽  
pp. 565-566
Author(s):  
Jiangtao Su ◽  
Yu Liu

AbstractIn this paper, we study twisting motions of the penumbral filaments of active region NOAA 10930. At first, they made unwinding motions. After unwinding, the filaments are found to twist again and developed the opposite chirality in them. These observational results indicate that penumbral filaments are more inclined to be the twisted magnetic flux tubes in nature.


2013 ◽  
Vol 51 (10) ◽  
pp. 1834-1841 ◽  
Author(s):  
Mariano Poisson ◽  
Marcelo López Fuentes ◽  
Cristina H. Mandrini ◽  
Pascal Démoulin ◽  
Etienne Pariat

2020 ◽  
Vol 36 (3) ◽  
pp. 69-90
Author(s):  
S. N. Chornogor ◽  
◽  
N. N. Kondrashova ◽  

2020 ◽  
Vol 60 (7) ◽  
pp. 936-941
Author(s):  
M. I. Savchenko ◽  
P. V. Vatagin ◽  
P. B. Dmitriev ◽  
M. G. Ogurtsov ◽  
E. M. Kruglov ◽  
...  

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