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Research Article Open access CC BY 4.0

Modeling Total Electron Content and Critical Frequency at F1 and E Layer Boundary

Kadidia Nonlo Drabo, Moustapha Konate, Roger Nakolemda, Gedeon Sawadogo, Emmanuel Nanéma, Frédéric Ouattara

Asian Journal of Physical and Chemical Sciences · pp. 37–42 · Published 5 Dec 2023

10.9734/ajopacs/2023/v11i4213

Abstract

This work investigates the variation of the total electron content TEC and the critical frequency fo in the boundary zone of the F1 and E layers at the low-latitude in the ionosphere. This study takes place at the Ouagadougou station (12.4°N and 358.5°E), in West Africa during the quiet geomagnetic activity of solar cycle 23. Ionosphere is the upper layer of the Earth's atmosphere ionized mainly by solar X- and UV-rays, extending from around 80km altitude up to 1000km [1] [2]. Ultraviolet light from the sun ionizes the atoms and molecules in the Earth's upper atmosphere [3]. For this study we use the 2016 version of International Reference Ionosphere (IRI) model. The quiet periods of maximum and minimum phase of solar cycle 23 are considered [4] [5]. From this study, it emerges that at the E and F1 layer boundary zone, TEC and fo increase during the day as solar irradiance increases and decrease as solar irradiance decreases.

Total electron content critical frequency maximum phase minimum phase quiet days

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