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International Letters of Chemistry, Physics and Astronomy
Volume 51
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Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection

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Abstract:

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.

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Periodical:
International Letters of Chemistry, Physics and Astronomy (Volume 51)
Pages:
26-33
Citation:
N. Husien et al., "Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection", International Letters of Chemistry, Physics and Astronomy, Vol. 51, pp. 26-33, 2015
Online since:
May 2015
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