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首页> 外文会议>International Cosmic Ray Conference >Study of coronal mass ejections along with solar and geomagnetic activity
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Study of coronal mass ejections along with solar and geomagnetic activity

机译：冠状大规模喷射以及太阳能和地磁活动的研究

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Co Coronal mass ejections are spectacular manifestations of solar activity in which 10+15 ronal –10+16 g of solar material are propelled outward into interplanetary space. Coronal Mass Ejections (CMEs) are large, energetic expu expul- lsions of mass and magnetic fields from t sions the Sun. CMEs can significantly affect large volume of the heliosphere and he appear to be a key cause of geomagnetic storms. CMEs cause depressions in the cosmic ray intensity both locally when an observer is inside the interplanetary structure and remotely i if the structure is energetic enough to create an f interplanetary shock to which the observer is magnetically connected. The goal of this study was to determine the di dis- stribution of various forms of solar activity that were spatially and temporally associated tribution with mass ejections during solar minimum phase. We have studied the influence of CMEs on solar and geomagnetic activity. It is noted that these CMEs do not produce significant effects on geomagnetic activity. The study suggests that maximum probability of geomagnetic disturbances occurs not on the onset of CME but after few days.
机译：CO冠状质量射出是太阳能活性的壮观表现，其中10 + 15 ronal -10 + 16g太阳能材料向外推进到行星际空间。冠状质量射入（CMES）是大，精力充沛的弥漫性暴露的群众和磁场从T分子太阳。 CMES可以显着影响大量的幽光圈，他似乎是地磁风暴的关键原因。当观察者在行星结构内部和远程I时，CMES在本地引起宇宙射线强度的凹陷，如果结构足够有能量以创建观察者被磁连接的F行星际冲击，则在其上远程。本研究的目的是确定在太阳最小相期间在空间和时间相关的各种形式的太阳能活性的不同形式的太阳能活性。我们研究了CME对太阳能和地磁活动的影响。注意，这些CME不会对地磁活动产生显着影响。该研究表明，几天后，几天后，几天的地磁干扰的最大概率不会发生。

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