1996 - 2019年磁层对流电场(MCEF)日变化特征:日冕物质抛射和磁云地球有效性特征的对比研究

Salfo Kaboré, Aristide Marie Frédéric Gyébré, Inza Gnanou, Frédéric Ouattara
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引用次数: 0

摘要

本文比较了1996 - 2019年地球有效行星际日冕物质抛射(ICMEs)引起的冲击活动和磁云对磁层对流电场(MCEF)日变化的特征。该研究是作为行星际磁场(IMF)方向的函数进行的。两种地磁活动的MCEF在时间上的变化是不同的,但都表现出对太阳周期相位的依赖。对于某一阶段,激波日MCEF的日平均值高于磁云日。同样,在任何时候,在相位最小和下降阶段,冲击日的每小时MCEF值都高于磁云活动日的每小时MCEF值。在所有阶段(无论哪个阶段)都观察到相同的结果。在相位最小时,在冲击日有夜间重连,而在磁云活动日,MCEF以一个向北的IMF结束一天。在相位极大时,这两种活动在地球磁层的裂片处都有磁重联。在下降阶段,(1)在激波活动的日子里,磁层叶重联(2)从1000 UT到2400 UT, IMF保持向南方向。关键词:磁层对流电场,行星际磁场,行星际日冕物质抛射,激波活动,磁云活动
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Diurnal variability of the magnetospheric convective electric field (MCEF) from 1996 to 2019: Comparative investigation into the signatures of the geoeffectiveness of coronal mass ejections and magnetic clouds
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来源期刊
Scientific Research and Essays
Scientific Research and Essays 综合性期刊-综合性期刊
自引率
0.00%
发文量
6
审稿时长
3.3 months
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