Growth of geomagnetic-induced currents during coronal mass ejection and corotating solar wind streams of geomagnetic storms in 2021

V. B. Belakhovsky; Белаховский В. Б.; V. A. Pilipenko; Пилипенко В. А.; Ya. A. Sakharov; Сахаров Я. А.; V. N. Selivanov; Селиванов В. Н.

doi:10.31857/S0367676522700478

Growth of geomagnetic-induced currents during coronal mass ejection and corotating solar wind streams of geomagnetic storms in 2021

Авторлар: Belakhovsky V.B.¹, Pilipenko V.A.², Sakharov Y.A.¹^,2, Selivanov V.N.³
Мекемелер:
1. Polar Geophysical Institute
2. Geophysical Center of the Russian Academy of Sciences
3. Northern Energetics Research Centre, Federal Research Centre “Kola Science Centre of the Russian Academy of Sciences”
Шығарылым: Том 87, № 2 (2023)
Беттер: 271-277
Бөлім: Articles
URL: https://cardiosomatics.ru/0367-6765/article/view/654488
DOI: https://doi.org/10.31857/S0367676522700478
EDN: https://elibrary.ru/AITPFO
ID: 654488

Дәйексөз келтіру

Толық мәтін

Ашық рұқсат
Рұқсат жабық

Рұқсат берілді
Рұқсат жабық

Тек жазылушылар үшін

Аннотация
Авторлар туралы
Әдебиет тізімі
Қосымша файлдар
Статистика

Аннотация

We analyzed the growth of geomagnetically induced currents (GIC) recorded in power lines on the Kola Peninsula during two types of magnetic storms: caused by the arrival of a coronal mass ejection (CME) and caused by a high-speed corotating solar wind stream (CIR). The relative efficiency of the CIR of the storm (the ratio of the maximum values of the GIC and the |Dst| index) turned out to be almost 3 times greater than that of the CME of the storm. This is caused by the large contribution of Pi3 geomagnetic pulsations and associated medium-scale vortex current systems in the ionosphere.

Әдебиет тізімі

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