Abstract
This article broadly reviews our knowledge of theoretical solar radio burst type III (SRBT III) in the low frequency region. The eruption mechanism of solar flares and type III are currently an extremely active area of research especially during the solar cycle is towards maximum. There is a particular focus on their physical properties, as opposed to the microphysics such as that needed for the evolution and formation of this burst or particle acceleration as such. In this work we summarize the related theory, model, significant parameters and relate it with the behavior of the burst in low range frequency. Although this is only a combination of all significant literature, it is hoped that it will give some idea on how to understand in details on this burst
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