*Suhaila M BUHARI1, Mardina ABDULLAH2, Alina marie HASBI3, Yuichi OTSUKA4, Michi NISHIOKA5, Takuya TSUGAWA5
(1.Physics Department, Universiti Teknologi Malaysia, 2.Space Science Centre, Universiti Kebangsaan Malaysia, 3.Department of Electrical, Electronics & Systems Engineering, Universiti Kebangsaan Malaysia, 4.Solar-Terrestrial Environment Laboratory, Nagoya University, 5.National Institute of Information and Communications Technology)
Keywords:equatorial plasma bubble, rate of TEC index, GPS TEC measurement
The equatorial plasma bubble (EPB) commonly occurs near the equatorial region after post sunset period. The generation process of EPB has been well understood where it is commonly developed near the magnetic equator and elongated along magnetic field lines through Rayleigh-Taylor instability mechanism. However, the source of seeding perturbation leads to the generation of Rayleigh-Taylor instability is still unknown. The temporal and spatial properties of EPB have been well studied using airglow imager. However, the observation using airglow imager is impossible during sunset time where the EPB starts to develop due to light from the sun while the observation during night time is always interfered by moon and clouds. In this study, we obtain the GPS data from Malaysia Real-Time Kinematics GNSS Network (MyRTKnet), International Ground Station (IGS) network and Sumatera GPS Array (SUGAR) network. The networks contains 127 receivers in South East Asia (SEA) region covers 8oN to -8oS latitude and 92oE to 120oE longitude geographic coordinates. In this study, we detected the structure of EPB using two-dimensional map of rate of TEC index (ROTI) calculated from ground based GPS TEC measurement in. The average ROTI value for all visible satellites at 300 km altitude is binned into 0.45o x 0.45o grid in geographic latitude and longitude. The advantage of this technique is the GPS data is always available and we are able to observe the spatial and temporal properties of EPBs continuously without distracted by light.On the 17th March 2011, we observed the appearance of EPB structure pass through the SEA territory for 5 hours from 1300 UT (2100 LT) - 1900 UT (0200 LT). The initial ROTI-enhancement region is at 1300 UT is propagating to eastward direction and the information of the structure is lost due to the limited coverage of GPS receiver. At 1340 UT, a new ROTI-enhancement region appeared as a point source at geographic coordinate 2oN and 98oE as shown in Figure (a). After 20 minutes, the point source of ROTI-enhancement region expand to ~600 km in the North and ~200 km South direction as shown in Figure (b) while the zonal size ~50 km remains the same. The perturbation region is expanding faster towards dip magnetic equator might associated with field-aligned irregularities. The structure travelled in eastward direction with velocity ~133 ms-1 until the development process stopped. After 60 minutes, we assumed the structure is fully developed as illustrated in Figure (c) when no development in zonal size and ROTI value is observed anymore. The developed structure has 200 km zonal size continuously moves to eastward directions with slower velocity ~111 ms-1. The slower velocity incidentally with no development in zonal size and ROTI value might indicates the "fossil" bubble where the plasma density is equal with background density and the structure velocity following the background plasma density. At 1440 UT the second structure is coming ~600 km away from the first structure with velocity ~111 ms-1 and zonal size 200 km same as the previous structure as shown in Figure (d). The first and second structure has the same zonal sizes and velocities might due to the same temporal and spatial evolution during the generation process.The two-dimensional structure of EPB has been presented using GPS networks in SEA region is an alternative tool to observe the temporal and spatial properties of EPB structure from the initial perturbation until the decaying process without being distracted by light. The temporal and spatial properties of EPB can contribute towards understanding the generation mechanism of the Rayleigh-Taylor instability process.