Equatorial plasma bubbles (EPBs) are the irregularities in the post-sunset equatorial/low-latitude ionosphere, manifesting as spread-F in ionograms (Bekner & Wells, 1934), scintillations in radio signals (Whitney & Malik, 1968), bite-outs in ion-density measurements (Hanson & Sanatani, 1973), plume structures in radar maps (Woodman & La Hoz, 1976), and intensity depletions in airglow images (Weber et al., 1978). EPBs are initiated by Rayleigh-Taylor instability (Dungey, 1956) operating in the post-sunset bottom-side F-region where vertical plasma density gradient is anti-parallel to gravity, under favorable conditions of seed perturbations, sharper plasma density gradients, smaller ion-neutral collisions, and stronger vertical plasma drifts (Sultan, 1996). Several review articles discuss the history and progress in the theoretical and technical evolution of EPB monitoring (