Electromagnetic Emissions from the ZEVS Transmitter and Northern Power Transmission Line, Registered on the CSES Satellite

82 Hz radiation from the ZEVS transmitter and 50 Hz emissions from the Northern Transit power transmission line are registered by the low-orbit satellite CSES (altitude ∼500 km) while flying over the Kola Peninsula. The ZEVS signal is detected at distances of 300 to 2300 km, as measured between the subsatellite point and the transmitter. Amplitude of electric component |E| at frequency of 82 Hz is found to be around 2.5 µV/m at 800 km from the transmitter. The corresponding amplitude of magnetic component |B| is found to be around 1.3 pT. The spatial structure of amplitudes of 50 Hz radiation is rearranged dramatically during the satellite’s transition from one power line to another. The amplitude of the electric and magnetic components of 50 Hz radiation registered above the Northern Transit power line is estimated at |E| ≈ 0.5–2.0 µV/m and |B| ≈ 0.5–1.5 pT. Measurements at short distances from the source (several hundred km) agree qualitatively with the results on the modeled spatial structure of the wave field in the upper ionosphere, excited by a horizontal current of a finite length. However, the amplitude of the 82 Hz radiation fell along with distance from the ZEVS transmitter more slowly than in model calculations based on the assumption of a vertical geomagnetic field.

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Publication Details

Journal
Bulletin of the Russian Academy of Sciences Physics
Published
2025-05-01
DOI
https://doi.org/10.1134/s106287382571102x
Citations
3
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
3.46
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article

Electromagnetic Emissions from the ZEVS Transmitter and Northern Power Transmission Line, Registered on the CSES Satellite

Vyacheslav Pilipenko, N. G. Mazur, E. N. Fedorov, Shufan Zhao et al.
3 citations
Bulletin of the Russian Academy of Sciences Physics
Ionosphere and magnetosphere dynamics
3.46
article

Electromagnetic Emissions from the ZEVS Transmitter and Northern Power Transmission Line, Registered on the CSES Satellite

Vyacheslav Pilipenko, N. G. Mazur, E. N. Fedorov, Shufan Zhao, N.V. Savelyeva
article en
3 citations

Abstract

82 Hz radiation from the ZEVS transmitter and 50 Hz emissions from the Northern Transit power transmission line are registered by the low-orbit satellite CSES (altitude ∼500 km) while flying over the Kola Peninsula. The ZEVS signal is detected at distances of 300 to 2300 km, as measured between the subsatellite point and the transmitter. Amplitude of electric component |E| at frequency of 82 Hz is found to be around 2.5 µV/m at 800 km from the transmitter. The corresponding amplitude of magnetic component |B| is found to be around 1.3 pT. The spatial structure of amplitudes of 50 Hz radiation is rearranged dramatically during the satellite’s transition from one power line to another. The amplitude of the electric and magnetic components of 50 Hz radiation registered above the Northern Transit power line is estimated at |E| ≈ 0.5–2.0 µV/m and |B| ≈ 0.5–1.5 pT. Measurements at short distances from the source (several hundred km) agree qualitatively with the results on the modeled spatial structure of the wave field in the upper ionosphere, excited by a horizontal current of a finite length. However, the amplitude of the 82 Hz radiation fell along with distance from the ZEVS transmitter more slowly than in model calculations based on the assumption of a vertical geomagnetic field.

Bulletin of the Russian Academy of Sciences PhysicsVol. 89(5)
Chinese Academy of Sciences (CN), Space Research Institute (RU), National Space Science Center (CN), Schmidt Institute of Physics of the Earth (RU)
Affordable and clean energy
Openalex Percentile: Top 8%
Ionosphere and magnetosphere dynamics
3.46
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Electromagnetic Emissions from the ZEVS Transmitter and Northern Power Transmission Line, Registered on the CSES Satellite — Vyacheslav Pilipenko, N. G. Mazur, et al. · Bulletin of the Russian Academy of Sciences Physics (2025) | TGRS Research Map | TGRS