correlationbetweencontinuouslobereconnectioninthemidmagnetotailandsubstormexpansiononset
文献类型:期刊论文
作者 | ZHANG Hui1; PU Zuyin1; CAO Xin1; FU Suiyan1; XIAO Chijie2; LIU Zhenxing3; A Korth4; M Frazen4; ZONG Qiugong5; H Reme6 |
刊名 | chinesesciencebulletin
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出版日期 | 2006 |
卷号 | 51期号:22页码:2795 |
ISSN号 | 1001-6538 |
英文摘要 | Data on plasma sheet crossing measured by Cluster/HIA and Cluster/FGM during the period from July to October in 2001-2003 are analyzed. Based on previous work on the characteristic features of continuous lobe reconnection (CLR) described in reference, two case studies and a statistical analysis were carried out on correlation between CLR in the mid magnetotail and substorm expansion onset for the events occurring during this period. It is found that almost all CLR events are in close connection with substorms. The beginning of CLR is almost always a few minutes ahead of substorm activities seen in the near Earth magnetotail and on the ground-based stations. This provides a clear indication that CLR is the virtual cause of substorm expansion onset during the period of continuous southward interplanetary magnetic field. |
语种 | 英语 |
源URL | [http://ir.bao.ac.cn/handle/114a11/51681] ![]() |
专题 | 中国科学院国家天文台 |
作者单位 | 1.北京大学 2.中国科学院国家天文台 3.中国科学院 4.Max-Planck-Institute for Solar System Research 5.Center for Atmospheric Research, UML 6.CESR/CNRS, Toulouse F-31028 7.IGM, Braunschweig D-38106 8.Los Alamos National Laboratory 9.Rutherford Appleton Laboratory |
推荐引用方式 GB/T 7714 | ZHANG Hui,PU Zuyin,CAO Xin,et al. correlationbetweencontinuouslobereconnectioninthemidmagnetotailandsubstormexpansiononset[J]. chinesesciencebulletin,2006,51(22):2795. |
APA | ZHANG Hui.,PU Zuyin.,CAO Xin.,FU Suiyan.,XIAO Chijie.,...&M W Dunlop.(2006).correlationbetweencontinuouslobereconnectioninthemidmagnetotailandsubstormexpansiononset.chinesesciencebulletin,51(22),2795. |
MLA | ZHANG Hui,et al."correlationbetweencontinuouslobereconnectioninthemidmagnetotailandsubstormexpansiononset".chinesesciencebulletin 51.22(2006):2795. |
入库方式: OAI收割
来源:国家天文台
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