The Magnetic Helicity Budget of Solar Active Regions and Coronal Mass Ejections

2003 ◽  
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Author(s):  
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J. Zhang ◽  
H. Zhang
2010 ◽  
Vol 521 ◽  
pp. A56 ◽  
Author(s):  
A. Smyrli ◽  
F. Zuccarello ◽  
P. Romano ◽  
F. P. Zuccarello ◽  
S. L. Guglielmino ◽  
...  

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Y. Liu ◽  
J. T. Hoeksema ◽  
M. Bobra ◽  
K. Hayashi ◽  
P. W. Schuck ◽  
...  

Solar Physics ◽  
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Vol 223 (1-2) ◽  
pp. 39-55 ◽  
Author(s):  
Jongchul Chae ◽  
Yong-Jae Moon ◽  
Young-Deuk Park

2008 ◽  
Vol 41 (6) ◽  
pp. 893-896
Author(s):  
Piyali Chatterjee ◽  
Arnab Rai Choudhuri ◽  
Kristof Petrovay ◽  
Dibyendu Nandy

2012 ◽  
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Yu Gao ◽  
Hongqi Zhang ◽  
Takashi Sakurai ◽  
Masaoki Hagino ◽  
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2005 ◽  
Vol 13 ◽  
pp. 117-118 ◽  
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M. K. Georgoulis ◽  
B. J. LaBonte ◽  
D. M. Rust

AbstractWe introduce a method to calculate the magnetic helicity density in a given active-region vector magnetogram, and a lower limit of it, based on a linear force-free (Iff) approximation. Moreover, we provide a lower limit of the total magnetic helicity in the active region (AR). A time series of magnetograms can be used to calculate the rate of helicity transport. The results can be then correlated with manifestations of the dynamical activity in ARs, such as flares and filament eruptions.


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