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THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016

Coronal Mass Ejections (CMEs) have been studied has become the most important phenomena of solar activity because it is the most energetic phenomena on the Sun. Concerning the importance of the impact of solar radio burst, we study the selected event of CMEs to observe the environment of the atmosph...

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Main Authors: Roslan, Umar, Z. S., Hamidi, N. M., Shariff
Format: Article
Language:English
Published: 2018
Subjects:
QC Physics
Online Access:http://eprints.unisza.edu.my/6699/1/FH02-ESERI-18-13441.pdf
http://eprints.unisza.edu.my/6699/
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spelling my-unisza-ir.66992022-04-03T02:14:17Z http://eprints.unisza.edu.my/6699/ THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016 Roslan, Umar Z. S., Hamidi N. M., Shariff QC Physics Coronal Mass Ejections (CMEs) have been studied has become the most important phenomena of solar activity because it is the most energetic phenomena on the Sun. Concerning the importance of the impact of solar radio burst, we study the selected event of CMEs to observe the environment of the atmosphere of the Sun. It was found that the geomagnetic field was at active to severe storm conditions due to continued activity from the active region. The sunspot number is 76 and radio flux exceeds 92 sfu. There are eight sunspots and with a density of 2.9 proton/ cm 3 . During that event, solar wind also reached up to 540.6 kmsec -1 . It is recommended to collect data for 5 years and above in order to observe the trend of the graph between SRBT II and the speed of CMEs 2018-01 Article PeerReviewed text en http://eprints.unisza.edu.my/6699/1/FH02-ESERI-18-13441.pdf Roslan, Umar and Z. S., Hamidi and N. M., Shariff (2018) THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016. Journal of Fundamental and Applied Sciences, 10 (1S). pp. 352-363. ISSN 1112-9867
institution Universiti Sultan Zainal Abidin
building UNISZA Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Sultan Zainal Abidin
content_source UNISZA Institutional Repository
url_provider https://eprints.unisza.edu.my/
language English
topic QC Physics
spellingShingle QC Physics
Roslan, Umar
Z. S., Hamidi
N. M., Shariff
THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
description Coronal Mass Ejections (CMEs) have been studied has become the most important phenomena of solar activity because it is the most energetic phenomena on the Sun. Concerning the importance of the impact of solar radio burst, we study the selected event of CMEs to observe the environment of the atmosphere of the Sun. It was found that the geomagnetic field was at active to severe storm conditions due to continued activity from the active region. The sunspot number is 76 and radio flux exceeds 92 sfu. There are eight sunspots and with a density of 2.9 proton/ cm 3 . During that event, solar wind also reached up to 540.6 kmsec -1 . It is recommended to collect data for 5 years and above in order to observe the trend of the graph between SRBT II and the speed of CMEs
format Article
author Roslan, Umar
Z. S., Hamidi
N. M., Shariff
author_facet Roslan, Umar
Z. S., Hamidi
N. M., Shariff
author_sort Roslan, Umar
title THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
title_short THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
title_full THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
title_fullStr THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
title_full_unstemmed THE ENVIRONMENT OF THE SUN DURING THE EXPLOSION OF CORONAL MASS EJECTIONS (CMES) ON 2ND MAY 2016
title_sort environment of the sun during the explosion of coronal mass ejections (cmes) on 2nd may 2016
publishDate 2018
url http://eprints.unisza.edu.my/6699/1/FH02-ESERI-18-13441.pdf
http://eprints.unisza.edu.my/6699/
_version_ 1729708880705880064
score 13.214268

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