7–11 Jul 2025
University of the Witwatersrand, Johannesburg
Africa/Johannesburg timezone

Exploring Long-term trends in total electron content over South Africa.

8 Jul 2025, 15:00
20m
Solomon Mahlangu House (University of the Witwatersrand, Johannesburg)

Solomon Mahlangu House

University of the Witwatersrand, Johannesburg

Oral Presentation Track D2 - Space Science Astrophysics & Space Science

Speaker

Modiri Mokaila (North West University)

Description

The ionosphere is a dynamic, inhomogeneous and conductive plasma formed from the interaction of solar Extreme Ultraviolet (EUV) and X-ray radiation with the quasi-neutral atmosphere of the Earth, found at 60 – 1000 km above sea level. With different peak levels of ionization, it is predominantly studied by determining the total number of particles that pass through a square meter area between a ground-based station and a GPS satellite – Total Electron Content (TEC). The importance of TEC is owed by its effect in radio communication, position, telemetry and tracking. An abundance of free electron gas in the ionosphere causes a delay of signals in the radio band. This study explores the long-term trends in TEC over South Africa at 2 GPS stations located 1000 km apart. TEC was computed using the IONOLAB software over SUTH and HRAO stations for a period of 25 years. The TEC trend analysis was performed using 3 solar proxies (sunspot numbers, MgII and F10.7). Preliminary results show a negative TEC trend between 1998 and 2023 over these mid-latitudes stations in South Africa. This is consistent with related global studies reported in the literature.

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Primary author

Modiri Mokaila (North West University)

Co-authors

Prof. Daniel M. Moeketsi (Centre for Space Research, North-West University) Prof. John Bosco Habarulema (South African National Space Agency (SANSA))

Presentation materials

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