| _version_ |
1860796911990079488
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| building |
INTELEK Repository
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| collection |
Online Access
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| collectionurl |
https://intelek.unisza.edu.my/intelek/pages/search.php?search=!collection407072
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| date |
2021-03-22 02:53:20
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| eventvenue |
Selangor, Virtual
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| format |
Restricted Document
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| id |
10656
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| institution |
UniSZA
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| originalfilename |
4725-01-FH03-ESERI-21-51642.pdf
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| person |
Mozilla/5.0 (Windows NT 6.1; Win64; x64) AppleWebKit/537.36 (KHTML
like Gecko) Chrome/88.0.4324.190 Safari/537.36
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| recordtype |
oai_dc
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| resourceurl |
https://intelek.unisza.edu.my/intelek/pages/view.php?ref=10656
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| spelling |
10656 https://intelek.unisza.edu.my/intelek/pages/view.php?ref=10656 https://intelek.unisza.edu.my/intelek/pages/search.php?search=!collection407072 Restricted Document Conference Conference Paper application/pdf 4 1.6 Mozilla/5.0 (Windows NT 6.1; Win64; x64) AppleWebKit/537.36 (KHTML like Gecko) Chrome/88.0.4324.190 Safari/537.36 Skia/PDF m88 2021-03-22 02:53:20 4725-01-FH03-ESERI-21-51642.pdf UniSZA Private Access Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event. Space weather is driven by solar activities by pulling out the variety of phenomenon such as solar flare and coronal mass ejection (CMEs). It been discovered the CMEs and solar flares have causes disturbance at near-Earth space. This paper is to examined the behaviour of geomagnetic storm, horizontal geomagnetic field and several solar wind parameters during solar flare and CMEs event at minimum of solar cycle of 24. Observational result found that association of strongest solar flare and CMEs have declined the geomagnetic storm until-150nt at 8th September 2017. Following to this, the H component reading also slightly decreased at three magnetometer location respectively. Solar flare and CMEs released the energetic particles that could disturbed the radio communications at the Earth and electronic equipment. Therefore, it was required to study and understanding the solar flare and CMEs event. 2nd International Conference on Space Weather and Satellite Application Selangor, Virtual
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| spellingShingle |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
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| summary |
Space weather is driven by solar activities by pulling out the variety of phenomenon such as solar flare and coronal mass ejection (CMEs). It been discovered the CMEs and solar flares have causes disturbance at near-Earth space. This paper is to examined the behaviour of geomagnetic storm, horizontal geomagnetic field and several solar wind parameters during solar flare and CMEs event at minimum of solar cycle of 24. Observational result found that association of strongest solar flare and CMEs have declined the geomagnetic storm until-150nt at 8th September 2017. Following to this, the H component reading also slightly decreased at three magnetometer location respectively. Solar flare and CMEs released the energetic particles that could disturbed the radio communications at the Earth and electronic equipment. Therefore, it was required to study and understanding the solar flare and CMEs event.
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| title |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
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| title_full |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
|
| title_fullStr |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
|
| title_full_unstemmed |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
|
| title_short |
Behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and CMEs event.
|
| title_sort |
behaviour of geomagnetic storm, horizontal geomagnetic field and solar wind parameters during solar flare and cmes event.
|