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摘要:
The coronal mass ejections (CMEs) produce by Sun poloidal magnetic fields contribute to geomagnetic storms. The geomagnetic storm effects produced by one-day-shock, two-days-shock and three-days-shock activities on Ouagadougou station F2 layer critical frequency time variation are analyzed. It is found that during the solar minimum and the increasing phases, the shock activity produces both positive and negative storms. The positive storm is observed during daytime. At the solar maximum and the decreasing phases only the positive storm is produced. At the solar minimum there is no three-days-shock activity. During the solar increasing phase the highest amplitude of the storm effect is due to the one-day-shock activity and the lowest is produced by the two-days-shock activity. At the solar maximum phase the ionosphere electric current system is not affected by the shock activity. Nevertheless, the highest amplitude of the storm effect is caused by the two-days-shock activity and the lowest by the one-day-shock activity. During the solar decreasing phase, the highest amplitude provoked by the storm is due to the three-days-shock activity and the lowest by the one-day-shock activity.
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篇名 The Geomagnetic Effects of Solar Activity as Measured at Ouagadougou Station
来源期刊 天文学与天体物理学国际期刊(英文) 学科 医学
关键词 CMES ACTIVITY Shock ACTIVITY F2 Layer Critical Frequency GEOMAGNETIC ACTIVITY IONOSPHERE Time Variation
年,卷(期) 2018,(2) 所属期刊栏目
研究方向 页码范围 178-190
页数 13页 分类号 R73
字数 语种
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研究主题发展历程
节点文献
CMES
ACTIVITY
Shock
ACTIVITY
F2
Layer
Critical
Frequency
GEOMAGNETIC
ACTIVITY
IONOSPHERE
Time
Variation
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研究来源
研究分支
研究去脉
引文网络交叉学科
相关学者/机构
期刊影响力
天文学与天体物理学国际期刊(英文)
季刊
2161-4717
武汉市江夏区汤逊湖北路38号光谷总部空间
出版文献量(篇)
333
总下载数(次)
0
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0
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