Low‐Latitude Zonal Ion Drifts and Their Relationship with Subauroral Polarization Streams and Auroral Return Flows during Intense Magnetic Storms

Author(s):  
Chao‐Song Huang ◽  
Yongliang Zhang ◽  
Wenbin Wang ◽  
Dong Lin ◽  
Qian Wu
2000 ◽  
Vol 27 (13) ◽  
pp. 1851-1854 ◽  
Author(s):  
C. G. Fesen ◽  
G. Crowley ◽  
R. G. Roble ◽  
A. D. Richmond ◽  
B. G. Fejer
Keyword(s):  

2013 ◽  
Vol 118 (6) ◽  
pp. 3866-3876 ◽  
Author(s):  
G. D. Earle ◽  
R. L. Davidson ◽  
R. A. Heelis ◽  
W. R. Coley ◽  
D. R. Weimer ◽  
...  
Keyword(s):  

Radio Science ◽  
1993 ◽  
Vol 28 (3) ◽  
pp. 389-400 ◽  
Author(s):  
D. R. Lakshmi ◽  
R. S. Dabas ◽  
B. C. N. Rao ◽  
B. M. Reddy

1994 ◽  
Vol 46 (3) ◽  
pp. 231-252 ◽  
Author(s):  
K. Shiokawa ◽  
K. Yumoto ◽  
Y. Tanaka ◽  
T. Oguti ◽  
Y. Kiyama
Keyword(s):  

2021 ◽  
Vol 73 (1) ◽  
Author(s):  
Yusuke Ebihara ◽  
Shinichi Watari ◽  
Sandeep Kumar

AbstractLarge-amplitude geomagnetically induced currents (GICs) are the natural consequences of the solar–terrestrial connection triggered by solar eruptions. The threat of severe damage of power grids due to the GICs is a major concern, in particular, at high latitudes, but is not well understood as for low-latitude power grids. The purpose of this study is to evaluate the lower limit of the GICs that could flow in the Japanese power grid against a Carrington-class severe magnetic storm. On the basis of the geomagnetic disturbances (GMDs) observed at Colaba, India, during the Carrington event in 1859, we calculated the geoelectric disturbances (GEDs) by a convolution theory, and calculated GICs flowing through transformers at 3 substations in the Japanese extra-high-voltage (500-kV) power grid by a linear combination of the GEDs. The estimated GEDs could reach ~ 2.5 V/km at Kakioka, and the GICs could reach, at least, 89 ± 30 A near the storm maximum. These values are several times larger than those estimated for the 13–14 March 1989 storm (in which power blackout occurred in Canada), and the 29–31 October 2003 storm (in which power blackout occurred in Sweden). The GICs estimated here are the lower limits, and there is a probability of stronger GICs at other substations. The method introduced here will be immediately applicable for benchmark evaluation of low-latitude GICs against the Carrington-class magnetic storms if one assumes electrical parameters, such as resistance of transmission lines, with sufficient accuracy.


1989 ◽  
Vol 94 (A6) ◽  
pp. 6751-6761 ◽  
Author(s):  
W. R. Coley ◽  
R. A. Heelis
Keyword(s):  

2018 ◽  
Author(s):  
Hisashi Hayakawa ◽  
José M. Vaquero ◽  
Yusuke Ebihara

Abstract. While low latitude auroral displays are normally considered to be a manifestation of magnetic storms of considerable size, Silverman (2003, JGR, 108, A4) reported numerous sporadic auroras which appear locally at relatively low magnetic latitudes during times of just moderate magnetic activity. Here, a case study is presented of an aurora near the geomagnetic equator based on a report from the Philippine Islands on 27 October 1856. An analysis of this report shows it to be consistent with the known cases of sporadic aurorae except for its considerably low magnetic latitude. The record also suggests that extremely low-latitude aurora is not always accompanied with large magnetic storms. The description of its brief appearance leads to a possible physical explanation based on an ephemeral magnetospheric disturbance provoking this sporadic aurora.


2018 ◽  
Vol 36 (4) ◽  
pp. 1153-1160 ◽  
Author(s):  
Hisashi Hayakawa ◽  
José M. Vaquero ◽  
Yusuke Ebihara

Abstract. While low-latitude auroral displays are normally considered to be a manifestation of magnetic storms of considerable size, Silverman (2003, JGR, 108, A4) reported numerous “sporadic auroras” which appear locally at relatively low magnetic latitude during times of just moderate magnetic activity. Here, a case study is presented of an aurora near the geomagnetic equator based on a report from the Philippine islands on 27 October 1856. An analysis of this report shows it to be consistent with the known cases of sporadic auroras, except for its appearance at considerably low magnetic latitude. The record also suggests that an extremely low-latitude aurora is not always accompanied by large magnetic storms. The description of its brief appearance leads to a possible physical explanation based on an ephemeral magnetospheric disturbance provoking this sporadic aurora.


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