  Currently, our understanding of magnetic fields in exoplanets remains limited
compared to those within our solar system. Planets with magnetic fields emit
radio signals primarily due to the Electron Cyclotron Maser Instability
mechanism. In this study, we explore the feasibility of detecting radio
emissions from exoplanets using the Square Kilometre Array (SKA) radio
telescope. Utilizing data from the NASA Exoplanet Archive, we compile
information on confirmed exoplanets and estimate their radio emissions using
the RBL model. Our analysis reveals that three exoplanets- Qatar-4 b, TOI-1278
b, and WASP-173 A b- exhibit detectable radio signals suitable for observation
with the SKA telescope.
