EGU26-5749, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-5749
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 14:00–15:45 (CEST), Display time Tuesday, 05 May, 14:00–18:00
 
Hall X4, X4.88
Ground-Based PWING Observations of Power Line Harmonic Radiation in Finland During Geomagnetic Disturbances: Initial Results
Kristyna Drastichova1, Frantisek Nemec1, Kazuo Shiokawa2, Claudia Martinez-Calderon2, Jyrki Manninen3, and Tero Raita3
Kristyna Drastichova et al.
  • 1Charles University, Faculty of Mathematics and Physics, Department of Surface and Plasma Science, Prague, Czechia (kristyna.drastichova@gmail.com)
  • 2Nagoya University, Institute for Space-Earth Environmental Research, Nagoya, Japan
  • 3University of Oulu, Sodankylä Geophysical Observatory, Sodankylä, Finland

Power line harmonic radiation (PLHR) is an important anthropogenic source of electromagnetic waves generated by power networks. It appears at harmonic frequencies of the fundamental power grid frequency, and these harmonics can reach up to several thousand Hz. In this study, we analyse PLHR using wave measurements from the ground-based PWING network. This study primarily focuses on measurements conducted in northern Finland, specifically at Angeli (69.02°N, 25.82°E), Kannuslehto (67.74°N, 26.27°E), and Oulujarvi (64.51°N, 27.23°E). Wave intensity data with a high frequency resolution (1 Hz) are used to investigate the properties of PLHR from 50 Hz up to 1000 Hz, particularly its dependence on geomagnetically induced currents (GICs) associated with space weather events. The wave data are complemented by nearby 1 s magnetometer measurements from the Finnish IMAGE network stations, which are used to estimate GIC strength via the temporal variation of the horizontal magnetic field component (dB/dt). Preliminary results for geomagnetic storms of October 2024 and January 2025 indicate that the intensity of PLHR is significantly enhanced by an order of magnitude during geomagnetic active times, particularly for even harmonics at 300 Hz, 600 Hz, and 900 Hz, which are usually weak or absent in well-operating power systems and appear mostly when the current waveform gets distorted. We also investigate a possible delay between GIC events and the resulting distortion of the current waveforms, and discuss the implications for the required time resolution of magnetometer data.

How to cite: Drastichova, K., Nemec, F., Shiokawa, K., Martinez-Calderon, C., Manninen, J., and Raita, T.: Ground-Based PWING Observations of Power Line Harmonic Radiation in Finland During Geomagnetic Disturbances: Initial Results, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-5749, https://doi.org/10.5194/egusphere-egu26-5749, 2026.