Abstract The present study aims to investigate the behaviour of equatorial plasma bubbles (EPBs) during quiet days in Southeast Asia (SEA). The behaviour of EPB was determined by observing their number (n) and zonal drift velocity (VE) from 2011 to 2013. The variation of the n and VE during quiet days was investigated monthly and seasonally each year. Three networks which are Malaysia Real-Time Kinematics GNSS Network (MyRTKnet), Sumatran GPS Array networks (SuGAr) and International GNSS Service (IGS) in SEA that consists of 127 receivers were utilized to collect the high-density GPS data. The data were then used to generate the zonal keogram of the rate of total electron content index (ROTI) to estimate n and VE. From the observed data, there were 376 days characterized as geomagnetically quiet according to the Kp index, with a total of 2592 EPBs observed using ROTI keogram. The highest VE was found to be ∼126 m/s during the equinox, while the lowest was ∼65 m/s in December solstice. In addition, the maximum and minimum n throughout the period were 1937 during the equinox and 163 in December solstice, respectively. While a distinct diurnal pattern emerged for n throughout 2011 until 2013, a clear diurnal pattern of VE was only evident in 2013. This observation suggests a potential link between the year with a diurnal VE pattern and the continuous presence of EPB.
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