scholarly journals Correction to “Major geomagnetic storms (Dst≤ −100 nT) generated by corotating interaction regions”

2007 ◽  
Vol 112 (A12) ◽  
pp. n/a-n/a ◽  
Author(s):  
I. G. Richardson ◽  
D. F. Webb ◽  
J. Zhang ◽  
D. B. Berdichevsky ◽  
D. A. Biesecker ◽  
...  
Author(s):  
I. G. Richardson ◽  
D. F. Webb ◽  
J. Zhang ◽  
D. B. Berdichevsky ◽  
D. A. Biesecker ◽  
...  

Solar Physics ◽  
2008 ◽  
Vol 254 (2) ◽  
pp. 311-323 ◽  
Author(s):  
Yunhee Choi ◽  
Y.-J. Moon ◽  
Seonghwan Choi ◽  
Ji-Hye Baek ◽  
Sungsoo S. Kim ◽  
...  

Solar Physics ◽  
2021 ◽  
Vol 296 (8) ◽  
Author(s):  
Agnieszka Gil ◽  
Renata Modzelewska ◽  
Anna Wawrzaszek ◽  
Bozena Piekart ◽  
Tadeusz Milosz

AbstractThe solar rotation period is the most prominent mid-term periodicity in the temporal behaviour of solar, heliospheric, and geomagnetic parameters. It is also a cause of the repeatedly appearing geomagnetic storms originating from the corotating interaction regions (CIRs). Since geomagnetic CIR-driven storms have a natural periodic character, and geomagnetic storms impact energy infrastructure via geomagnetically induced currents, it is of interest whether this periodic character is also noticeable in the temporal behaviour of electrical-grid failures (EGFs), which, at least to some extent, might be of solar origin.


Solar Physics ◽  
2015 ◽  
Vol 290 (8) ◽  
pp. 2291-2309 ◽  
Author(s):  
T. M. Conlon ◽  
S. E. Milan ◽  
J. A. Davies ◽  
A. O. Williams

Solar Physics ◽  
2013 ◽  
Vol 285 (1-2) ◽  
pp. 201-216 ◽  
Author(s):  
J. A. Gonzalez-Esparza ◽  
E. Romero-Hernandez ◽  
P. Riley

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