Electric Current and Magnetic Shear in Solar Active Regions

2001 ◽  
Vol 557 (1) ◽  
pp. L71-L74 ◽  
Author(s):  
Hongqi Zhang
2017 ◽  
Vol 846 (1) ◽  
pp. L6 ◽  
Author(s):  
Yang Liu ◽  
Xudong Sun ◽  
Tibor Török ◽  
Viacheslav S. Titov ◽  
James E. Leake

2020 ◽  
Author(s):  
Tibor Torok ◽  
Yang Liu ◽  
James E. Leake ◽  
Xudong Sun ◽  
Viacheslav S. Titov

<p>The physical conditions that determine the eruptive activity of solar active regions (ARs) are still not well understood. Various proxies for predicting eruptive activity have been suggested, with relatively limited success. Moreover, it is presently unclear under which conditions an eruption will remain confined to the low corona or produce a coronal mass ejection (CME).</p><p>Using vector magnetogram data from SDO/HMI, we investigate the association between electric-current neutralization and eruptive activity for a sample of ARs. We find that the vast majority of CME-producing ARs are characterized by a strongly non-neutralized total current, while the total current in ARs that do not produce CMEs is almost perfectly neutralized, even if those ARs produce strong (X-class) confined flares. This suggests that the degree of current neutralization can serve as a good proxy for assessing the ability of ARs to produce CMEs. </p><p> </p>


1997 ◽  
Vol 482 (1) ◽  
pp. 519-534 ◽  
Author(s):  
D. A. Falconer ◽  
R. L. Moore ◽  
J. G. Porter ◽  
G. A. Gary ◽  
T. Shimizu

Solar Physics ◽  
1987 ◽  
Vol 109 (2) ◽  
pp. 307-320 ◽  
Author(s):  
Y. J. Ding ◽  
M. J. Hagyard ◽  
A. C. Deloach ◽  
Q. F. Hong ◽  
X. P. Liu

2012 ◽  
Vol 750 (1) ◽  
pp. 24 ◽  
Author(s):  
Ronald L. Moore ◽  
David A. Falconer ◽  
Alphonse C. Sterling

Sign in / Sign up

Export Citation Format

Share Document