ABSTRACT
A model is proposed in this paper that could predict the onset of Coronal Mass Ejection with a lead-time longer than 72 hours. This model appears to be able to give both the location on the surface of the sun and the time of the ejection. Coronal Mass Ejections (CMEs) may be described as a blast of gas and highly charged solar mass fragmets ejected into space. These ejections, when directed toward Earth, have manifold effects on terrestrial systems ranging from producing the Aurora Borealis to changes in wireless communications and in some cases disruption of power grids. The importance of an early prediction of these solar events cannot be ignored. There are several models currently utilized to predict these events. Prediction of both event and the location on the sun where the event will occur allows us to make some preparation for the event. This paper proposes a better preduction by utilizing low angular resulotion radio telescope arrays to catalog data from the sun at different radio frequencies on a regular basis. Once these data are cataloged a better predictor for these CMEs can be found.