2022
DOI: 10.1134/s0016793222060032
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Observations of Geomagnetic Induced Currents in Northwestern Russia: Case Studies

Abstract: We analyzed intense geomagnetically induced currents (GICs) recorded during a complex space weather event observed on 23-24 April 2023. Two geomagnetic storms characterized by SYM-H intensities of -179 nT and -233 nT was caused by southward IMF Bz of -25 nT in the sheath fields and -33 nT in the magnetic cloud (MC) fields. GIC observations were divided into two local time sectors: nighttime (1700-2400 UT on 23 April) GICs observed during the interplanetary sheath magnetic storm, and morning sector (0200-0700 U… Show more

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Cited by 7 publications
(4 citation statements)
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References 57 publications
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“…We contend that the high‐latitude vortices, low‐latitude substorm indicators, and the sub‐auroral G1‐G4 disturbance in the Mäntsälä pipeline were latitude‐spanning effects of a series of mesoscale flow injections or impingements. Minor timing differences can be attributed to the difference in overhead currents, ground and material conductivity, system configurations, and the north‐south orientation of the powerline (Despirak et al., 2022).…”
Section: Discussionmentioning
confidence: 99%
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“…We contend that the high‐latitude vortices, low‐latitude substorm indicators, and the sub‐auroral G1‐G4 disturbance in the Mäntsälä pipeline were latitude‐spanning effects of a series of mesoscale flow injections or impingements. Minor timing differences can be attributed to the difference in overhead currents, ground and material conductivity, system configurations, and the north‐south orientation of the powerline (Despirak et al., 2022).…”
Section: Discussionmentioning
confidence: 99%
“…From 15:56 to 16:04 UT on the Mäntsälä pipeline, the minimum‐to‐peak GIC variation was 22 A; in the same interval, there was a 70 A variation at Vykhodnoi power station in the Kola Peninsula. Figure 8c displays the currents for 16:04 UT (G1b) and shows an intense poleward current channel over the north end of the pipeline and the Kola peninsula, where strong ground magnetic fluctuations were observed (Belakhovsky et al., 2019; Despirak et al., 2022). The narrow current channel, bracketed by up‐down FACs (Figure 8c) and a poleward displacement of the R1‐FAC (Figure 6d) are consistent with the description of auroral streamer development during arrival of plasma flow bursts (e.g., Hubert et al., 2007; Zou et al., 2022).…”
Section: Discussionmentioning
confidence: 99%
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