Study of Equatorial Ionospheric Scintillation and TEC characteristics at Solar minimum using GPS-SCINDA data

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This paper presents a study of ionospheric scintillation and the Total Electron Content (TEC) characteristics at low solar activity using GPS data from a West African location.The data used are the scintillation index (S4) and the vertical TEC (vTEC) recorded at the GPS - SCINDA station of Abidjan (Latitude = 5.340 N, Longitude = 3.900 W). This work covers the period from January 2008 to January 2009.The results show that the scintillation is not intense with S4 values lower than 1 in most of the cases and during the course of the day. However from 2000 to 0200 local time, there are relatively high values of S4 confirming that scintillation is primarily a nighttime observed phenomenon. The scintillation shows a seasonal effect characterized by intense values in the equinoctial months compare to that of the solstice season. The vTEC in general exhibits a diurnal variation as a function of the solar zenith angle. Higher vTEC values are observed around 1500 local time and have the same seasonal variation with the S4 index.

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