NAOC Open IR
尾瓣持续磁重联与磁层亚暴相关性研究
濮祖荫1; 曹馨1; 傅绥燕1; 肖池阶2; 刘振兴3; A Korth4; M Frazen4; Q G Zong5; H Reme6; K H Glassmeier7; R Friedel8; G D Reeves8; M W Dunlop9; 张辉1
2006
Source Publication科学通报
ISSN0023-074X
Volume51Issue:4Pages:459
Abstract根据尾瓣持续磁重联的特征,首先利用Cluster星簇测量的近地磁尾等离子体密度、温度、整体运动速度、磁场等数据,确认尾瓣磁重联过程的存在;其次,利用GOES,LANL等同步高度卫星数据,极光数据以及地面观测的AE指数等描述亚暴突发(onset)现象;结合上述两方面的观测,进而分析研究了尾瓣持续磁重联和磁层亚暴的相关性和时序关系,确认了尾瓣持续磁重联是行星际磁场持续南向期间亚暴膨胀相突发的原因.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/48227
Collection中国科学院国家天文台
Affiliation1.北京大学
2.中国科学院国家天文台
3.中国科学院国家空间科学中心
4.Max-Planck-Institute for Solar System Research
5.波士顿大学
6.CESR/CNRS
7.IGM,TU Braunschweig
8.Los Alamos National Laboratory
9.Rutherford Appleton Laboratory
Recommended Citation
GB/T 7714
濮祖荫,曹馨,傅绥燕,等. 尾瓣持续磁重联与磁层亚暴相关性研究[J]. 科学通报,2006,51(4):459.
APA 濮祖荫.,曹馨.,傅绥燕.,肖池阶.,刘振兴.,...&张辉.(2006).尾瓣持续磁重联与磁层亚暴相关性研究.科学通报,51(4),459.
MLA 濮祖荫,et al."尾瓣持续磁重联与磁层亚暴相关性研究".科学通报 51.4(2006):459.
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