Open AccessThe Analysis of Solar Radio Burst Type III Associated with Solar Activities Due to Magnetic Reconnection from 2012-2017
Author(s) -
Zety Sharizat Hamidi,
N.N.M. Shariff
Publication year - 2020
Publication title -
journal of physics. conference series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.21
H-Index - 85
eISSN - 1742-6596
pISSN - 1742-6588
DOI - 10.1088/1742-6596/1593/1/012025
Subject(s) - solar flare , solar radio , physics , magnetic reconnection , coronal mass ejection , solar maximum , flux (metallurgy) , astrophysics , correlation coefficient , magnetic flux , solar wind , magnetic field , statistics , chemistry , mathematics , quantum mechanics , organic chemistry
Solar Radio Bursts Type III (SRBT III) and their correlation with solar flares always had been interesting issues. The objective of this research is to study the correlation of SRBT III related to solar flares to magnetic reconnection theory. The importance of this correlation is to enhance the understanding of the particles behaviour during the events over this burst. The data for both SRBT III can be obtained from the e - CALLISTO website. Meanwhile, the data for solar flares were obtained from the Solar Monitor website and Computer Aided CMEs Tracking website respectively. There are 44 data have been collected starting from 2012 until 2017. The Pearson Correlation Coefficient is a method used in obtaining the correlation of the variables of SRBT III and solar flares events. The value of R obtained for the peak flux and the starting frequency of SRBT III is +0.3364. The mean of the peak flux is 6.0 × 10 −5 W/m 2 which is in the M group with a magnitude of 6.0. From this study, they found that the single SRBT III is due to the single magnetic reconnection whereas for the storm and group SRBT III is due to the multiple magnetic reconnections.