Frontiers in Astronomy and Space Sciences· 2026Q2
Characterization of thunderstorm-generated travelling ionospheric disturbances by dense GNSS sensors network over Western Europe
- 1citations
- Q2SCImago
- 2026year
Short summary
Thunderstorms generate quasi-periodic travelling ionospheric disturbances (TIDs) that propagate up to 1000 km with speeds of 100-160 m/s and periods of 13-39 min, observable in total electron content (TEC) for many hours.
AI-generated from the title and abstract; the full text is not read.
Key points
- Thunderstorms generate quasi-periodic TIDs propagating circularly up to 1000 km.
- TIDs exhibit apparent horizontal phase speeds of 100-160 m/s and periods of 13-39 min.
- Wavelengths of 200-300 km and non-isotropic radiation patterns were observed for some storms.
- TIDs from storms may be masked by other ionospheric phenomena, like the solar terminator.
AI-generated from the title and abstract; the full text is not read.
Abstract
We used total electron content (TEC) measurements from 1200 ground-based GNSS receivers in Europe to study ionospheric effects of five convective storms that occurred between 2019 and 2024. The storms are of different types of activity by the meteorological classification (derecho, thunderstorm with sprites, Mediterranean storm, cold drop, ex-tropical storm “ex-Kirk), and are characterized by a stationary or a moving convective zone (thunderstorm). In all cases, we observe quasi-periodic travelling ionospheric disturbances (TIDs) propagating nearly circularly from the center of the storms, for up to 1000 km of distance, and they are visible in TEC for many hours. The apparent horizontal phase speeds are found between 100 m/s to 160 m/s. The TIDs periods range from 13 min to 39 min. These characteristics are consistent with previous observations and theoretical results. For three out of the five storms, the temporal evolution of the waves could be clearly mapped, enabling the measurement of a wavelength of around 200–300 km and a non-isotropic radiation pattern according to the propagation directions, as predicted by the models. Our analysis also demonstrates that these TIDs might not be visible in TEC during the presence of TIDs of other origins, e.g., the solar terminator.
The authors' abstract, as published at the source. Frontiers in Astronomy and Space Sciences, 2026 · DOI ↗
Continue with a free account
Ask the paper: 3 free questions a day about this paper; save it, get its citation, new summaries every day for your field. Takeaways are Premium.
Continue free on the webSign in with Google or Apple; no card needed. You come back to this paper.
On your phone:
Field: Astronomy and Astrophysics
Astronomy and AstrophysicsPhysics and Astronomy