Probability of Reception of Jovian Bursts as Derived from Io-Phase and the Location of Central Meridian Longitude

A radio telescope consisting of a receiver and a dual dipole antenna has been installed at high altitude station Darjeeling to detect solar and Jovian emissions at 20.1 MHz for receiving radio signal from both the Sun and the Jupiter. Signals received during September 2012 are analyzed to compare the Jovian bursts observed in predicted emission phases for the satellite Io of the Jupiter and the locations of CML, suggesting that the chances to record a burst in Io-phase is significantly large and even may be double than that in general CML locations.