Preliminary Analysis on the Solar Burst Type III and the Effect of the Magnetic Reconnection
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Date
2015
Publication Type
Journal Article
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yes
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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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published
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Book title
Volume
51
Pages / Article No.
26 - 33
Publisher
Scientific Publishing House Darwin
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Subject
Sun; solar burst; III; radio region; X-ray region; solar flare; active region
Organisational unit
03928 - Refregier, Alexandre / Refregier, Alexandre