ABSTRACT
During solar activity the energy particles of the sun released due to solar flare, Coronal Mass
Ejections (CMEs), coronal heating as well as sunspot. Solar radio burst will be observed in the
presence of solar activity such solar flare, CMEs and solar prominence as the indicator for those
events to happen. During the peak of solar cycle, the filaments are present due to the active magnetic
field and solar storm’s explosion. This type of solar radio burst normally can be seen in the phase of
impulsive solar flare. Therefore, it is crucial to understand field line connectivity in flare and the
access of flare accelerated particle to the earth. In this study, we highlighted on the observation of
solar radio burst type III on 9th of May at 05:31 UT till 05:44 UT. The event was successfully recoded
by e-CALLISTO using BLEINSW radio telescope. The Solar Radio Burst Type III that had been
observed was related to the Coronal Mass Ejections and the mechanisms that trigger the events have
been discussed. It is shown that the CMEs is believed to happen because of the magnetic filament that
connected to active region (AR) 2339 was erupted, and combination of two wild filament produced a
bright CMEs. Fortunately, the expanding cloud does not appear to be heading for earth.
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