Nurulhazwani Husien, Zety Sharizat Hamidi, N.N.M. Shariff, C. Monstein, Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection, ILCPA Volume 51, International Letters of Chemistry, Physics and Astronomy (Volume 51)
    From the data from a BLEIN Callisto site, we aim to provide a comprehensive description of the synopsis formation and dynamics of a a single solar burst type III and magnetic reconnection effect. The data above is the solar radio burst type iii occurred on 10th September 2005 between 05:44 UT till 06:00 UT.This eruption has started since 5:55 UT with a formation of type III solar burst. The wave emission process of solar radio burst type III from magnetic reconnection region in a solar flare were investigated by using a two-dimensional, that are electromagnetic and relativistic particle-in-cell code. The solar radio burst type III initially impose into two plasma populations : background dense plasma and hot electrons that can be generated by the magnetic reconnection process in a solar flare. The conversion of the energy stored in the magnetic field by a process called the magnetic reconnection released the energy in the solar flares and related phenomena. By the launching the e-CALLISTO network, its prove the existence of the magnetic reconnection on the surface of the sun in radio region.
    Active Region, III, Radio Region, Solar Burst, Solar Flare, Sun, X-Ray Region