NSSC OpenIR  > 空间科学部
Alternative TitleThe statistical characteristics of the tailward flows in the near-Earth region explored by TC-1
刘振兴; 张灵倩; 马志为; 王继业; 濮祖荫; 沈超; 郭九苓; 北京8701信箱
Source Publication地球物理学报
Keyword近地磁尾 尾向流 等离子体片 等离子体片边界层
Other AbstractDuring quiet time and substorm process,tailward flow often explored in the near-Earth magnetotail by TC-1 satellite.The tailward flow is most strong near the equator,and stronger in the dusk-side and dawn-side than that in the night-side.The tailward flow tends to move from the dusk-side and dawn-side to the night-side,and becomes stronger while moving away the Earth.From 1,Jul.2004 to 31,Nov.2004,TC-1 satellite explored 516 tailward flow events between 7 RE to 13 RE,which the duration exceed 3 min.The statistic results showed that:Compared with the earward flow from the mid-tail,the near2Earth low latitude tailward flow from the ionosphere is characteristic of the low-temperature and high density ; With the tailward flow moving from the lobal region to the plasma sheet,the velocity of the tailward flow decrease.the density and the temperature increase.The tailward flow has distinct anisotropy depending on the difference of the parallel with perpendicular temperature.
Indexed ByCSCD
Funding Project中国科学院空间科学与应用研究中心
Citation statistics
Cited Times:2[CSCD]   [CSCD Record]
Document Type期刊论文
Corresponding Author北京8701信箱
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GB/T 7714
刘振兴,张灵倩,马志为,等. 探测一号卫星在近地磁尾观测到的尾向流统计特性[J]. 地球物理学报,2007,50(3):655-661.
APA 刘振兴.,张灵倩.,马志为.,王继业.,濮祖荫.,...&北京8701信箱.(2007).探测一号卫星在近地磁尾观测到的尾向流统计特性.地球物理学报,50(3),655-661.
MLA 刘振兴,et al."探测一号卫星在近地磁尾观测到的尾向流统计特性".地球物理学报 50.3(2007):655-661.
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