Localized plasma density reduction in the F region at the equator is known as the equatorial plasma bubbles (EPBs). Notably, the zonal electric fields act as the primary controller of the EPB generation (Chakrabarty et al., 2006). In the F regions, the neutral winds blowing across the magnetic field lines create an electric field (dynamo action) (Heelis et al., 1974;Rishbeth et al., 1972). An early study by Rishbeth (1971) revealed that the zonal neutral winds in the equatorial F region that blow across the magnetic field can cause a slow transverse ion drift perpendicular to both the neutral wind and magnetic field, resulting in a polarized electric field which is directed vertically downwards. This downward electric field causes a plasma drift in the eastward direction, the same direction as the neutral wind. During the nighttime, the ionosphere becomes unstable because the plasma density gradient is upward and the ionospheric current flows eastward. At sunset, the equatorial F2 layer undergoes a fast rise due to the enhancement of the eastward electric field, called pre-reversal enhancement (PRE) causing upward plasma E × B drift (Fesen et al., 2000). Additionally, Woodman (1970) stated that PRE which is a sharp upward spike of the vertical ion velocities that occurs immediately after local sunset is a unique feature in the low-latitude ionosphere. EPBs usually occur right after the occurrence of PRE (Fesen et al., 2000;Heelis et al., 1974), suggesting that PRE plays an important role in EPB generation. However, EPB occurrences vary from day-to-day (Sharma et al., 2014). This phenomenon has been extensively investigated for decades using various equipment such as the incoherent back scatter radar, all-sky imager and satellites (