X lines in the magnetotail for southward and northward IMF conditions
文献类型:期刊论文
作者 | Zhang, L. Q.; Wang, J. Y.; Baumjohann, W.; Reme, H.; Dai, L.; Dunlop, M. W.; Chen, T.; Huang, Y. |
刊名 | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
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出版日期 | 2015 |
卷号 | 120期号:9页码:7764-7773 |
关键词 | X line IMF condition solar wind substorm AE index |
ISSN号 | 2169-9380 |
通讯作者 | Zhang, LQ (reprint author), Chinese Acad Sci, Natl Space Sci Ctr, State Key Lab Space Weather, Beijing, Peoples R China. |
英文摘要 | Utilizing associated observations of Geotail and ACE satellites from the year of 1998 to 2005, we investigated the X lines in the near-Earth tail under different interplanetary magnetic field (IMF) conditions. The X lines are recognized by the tailward fast flows with negative B-z. Statistically, the X lines in the tail can be observed for southward as well as northward IMF, but more frequently observed for southward IMF. A typical case on 26 April 2005 showed clear evidence that the X line can occur for northward IMF while the geomagnetic activity is particularly quiet. Further analysis showed that the X line-related solar wind has stronger E-y and B-z components for southward than northward IMF. In addition, the X line-related geomagnetic activities are stronger for southward than northward IMF. |
收录类别 | SCI |
语种 | 英语 |
公开日期 | 2016-04-26 |
源URL | [http://ir.nssc.ac.cn/handle/122/5350] ![]() |
专题 | 国家空间科学中心_空间科学部 |
推荐引用方式 GB/T 7714 | Zhang, L. Q.,Wang, J. Y.,Baumjohann, W.,et al. X lines in the magnetotail for southward and northward IMF conditions[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2015,120(9):7764-7773. |
APA | Zhang, L. Q..,Wang, J. Y..,Baumjohann, W..,Reme, H..,Dai, L..,...&Huang, Y..(2015).X lines in the magnetotail for southward and northward IMF conditions.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,120(9),7764-7773. |
MLA | Zhang, L. Q.,et al."X lines in the magnetotail for southward and northward IMF conditions".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 120.9(2015):7764-7773. |
入库方式: OAI收割
来源:国家空间科学中心
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