Spatial scale of geomagnetic Pc5/Pi3 pulsations as a factor of their efficiency in generation of geomagnetically induced currents

• Published in: Earth, Planets and Space
• Main Authors: Yagova, Nadezda V, Pilipenko, Vyacheslav A, Sakharov, Yaroslav A, Selivanov, Vasily N
• Other Authors: Russian Science Foundation
• Format: Article in Journal/Newspaper
• Language: English
• Published: Springer Science and Business Media LLC 2021
• Subjects: Space and Planetary Science; Geology; Kil; Kola Peninsula; kola peninsula
• Online Access: http://dx.doi.org/10.1186/s40623-021-01407-2; https://link.springer.com/content/pdf/10.1186/s40623-021-01407-2.pdf; https://link.springer.com/article/10.1186/s40623-021-01407-2/fulltext.html

Abstract Geomagnetically induced currents (GICs) in a quasi-meridional power transmission line on the Kola Peninsula are analyzed during the intervals of Pc5/Pi3 (frequency range from 1.5 to 5 mHz) pulsations recorded at the IMAGE magnetometer network. We have analyzed GIC in a transformer at the terminal station Vykhodnoy ( $$68^{\circ }$$ 68 ∘ N, $$33^{\circ }$$ 33 ∘ E) during the entire year of 2015, near the maximum of the 24th Solar cycle. To quantify the efficiency of GIC generation by geomagnetic pulsations, a ratio between power spectral densities of GIC and magnetic field variations is introduced. Upon examination of the geomagnetic pulsation efficiency in GIC generation, the emphasis is given to its dependence on frequency and spatial scale. To estimate pulsation spatial scales in latitudinal and longitudinal directions, the triangle of stations KEV-SOD-KIL has been used. Large-scale pulsations (with a high spectral coherence, low phase difference, and similar amplitudes at latitudinally separated stations) are found to be more effective in GIC generation than small-scale pulsations. The GIC response also depends on the pulsation scale across the electric power line.