For around 50 years, a solar flare is among the activities of the Sun that has been evaluated and observed by scientists. The origin of the solar flare is from the sunspot associated with a solar burst. The solar burst can be break into 5 types. Long duration solar bursts have been investigated in this study. There are 15 selected dates that have been chosen from 2019 until 2020. Radio flux and sunspot numbers affiliated with long-duration solar bursts have been analyzed in this paper. As a result, the longest and the shortest solar burst that has been recorded is 535 minutes on 14/04/19 and 36 minutes on 21/03/19 respectively. The Sun is very important to be consistently observed because in rare cases, the flare is very strong and can affect the Earth’s magnetosphere.
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29 June 2021
PROCEEDINGS OF THE 2ND PHYSICS AND MATERIALS SCIENCE INTERNATIONAL SYMPOSIUM (PhyMaS 2.0)
27 January 2021
Shah Alam, Malaysia
Research Article|
June 29 2021
An analysis of a long duration solar burst with radio flux and sunspot number
W. M. A. W. Ismail;
W. M. A. W. Ismail
a)
1
Faculty of Applied Sciences, Universiti Teknologi MARA Shah Alam
, 40450, Shah Alam, Selangor, Malaysia
a)Corresponding author: [email protected]
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Z. S. Hamidi;
Z. S. Hamidi
b)
1
Faculty of Applied Sciences, Universiti Teknologi MARA Shah Alam
, 40450, Shah Alam, Selangor, Malaysia
2
Institute of Science, Universiti Teknologi MARA Shah Alam
, 40450 Shah Alam, Selangor, Malaysia
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N. N. M. Shariff
N. N. M. Shariff
c)
2
Institute of Science, Universiti Teknologi MARA Shah Alam
, 40450 Shah Alam, Selangor, Malaysia
3
Academy of Contemporary Islamic Studies (ACIS), Universiti Teknologi MARA Shah Alam
, 40450 Shah Alam, Selangor, Malaysia
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W. M. A. W. Ismail
1,a)
Z. S. Hamidi
1,2,b)
N. N. M. Shariff
2,3,c)
1
Faculty of Applied Sciences, Universiti Teknologi MARA Shah Alam
, 40450, Shah Alam, Selangor, Malaysia
2
Institute of Science, Universiti Teknologi MARA Shah Alam
, 40450 Shah Alam, Selangor, Malaysia
3
Academy of Contemporary Islamic Studies (ACIS), Universiti Teknologi MARA Shah Alam
, 40450 Shah Alam, Selangor, Malaysia
AIP Conf. Proc. 2368, 040006 (2021)
Citation
W. M. A. W. Ismail, Z. S. Hamidi, N. N. M. Shariff; An analysis of a long duration solar burst with radio flux and sunspot number. AIP Conf. Proc. 29 June 2021; 2368 (1): 040006. https://doi.org/10.1063/5.0058498
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