Abstract <p>Ionospheric variability due to solar flares has been studied at different latitudes during the solar cycle 24. In the course of this cycle 24 on September 6, 2017, two powerful and intense solar flares of class X2.2 and X9.3 were emitted by the Sun at 0857 UT and 1153 UT respectively. To examine the ionospheric response simultaneously at low, mid, and high latitudes, total electron content (TEC) values derived from Global Navigation Satellite System (GNSS) receivers were investigated during the solar flare of September 6, 2017, which are the most remarkable flare events during the solar cycle-24. Our observations show a noticeable enlargement in TEC at low, mid, and high-latitude stations. Further, the mean method has been used to investigate TEC variations due to solar flares at low, mid, and high latitudes and considered all PRN which has a one-to-one correlation with the time of solar flares. We describe our findings in the context of earlier research which examined the correlation between change in VTEC (DVTEC) and solar fluxes in X-class solar flares. The aim of this study is to minimize the latitudinal variability of total electron content (TEC) during such events, although the extent of TEC increase seems to be influenced by the class of the solar flare. The results exhibited that X-class flare effects were more pronounced at low latitudes in comparison to mid and high latitudes.</p>