Observation of the evolution of the 25th solar cycle by measuring the ionospheric delay using the GPS P3 method in southeastern BrazilGPS P3 method in southeastern Brazil

Authors

  • Fábio Yamada Brazilian Air Force
  • Luiz V. G. Tarelho National Institute of Metrology, Quality, and Technology – INMETRO, Duque de Caxias, RJ, Brazil
  • Mauro V. Lima National Institute of Metrology, Quality, and Technology – INMETRO, Duque de Caxias, RJ, Brazil

DOI:

https://doi.org/10.21014/actaimeko.v14i2.1969

Keywords:

GPS P3 method, ionosphere, ionospheric refraction, total electron content, TEC

Abstract

Ionospheric refraction generates time delay and signal fading in the electromagnetic signals, which can cause errors in the receiver. These errors can range from a few meters in location to total signal unavailability, depending on the ionisation level of the ionosphere plasma. The parameter to evaluate the behaviour of the ionosphere is the Total Electron Content (TEC). This article will present the relationship between the evolution of the number of sunspots of the 25th solar cycle and the Vertical TEC (VTEC) measurement made by a geodetic receiver in the city of Xerém (Brazil). We applied the GPS P3 method of time and frequency transfer to the observables of the receiver. Periods related to the year's seasons (summer and winter) were analysed since the beginning of the 25th solar cycle in 2019. The VTEC analysis characterises the behaviour of the ionosphere caused by the daily, annual, summer, and winter variations in the incidence of solar radiation in southeastern Brazil. Therefore, the analysis can correlate the ionospheric fluctuation with the number of monthly sunspots, referring to the evolution of the 25th solar cycle. The findings of this study are expected to contribute to further developments of a deeper understanding of the ionosphere’s dynamics and further advancements in GNSS-related services.

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Published

2025-06-26

Issue

Section

Research Papers