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Characteristics of dayside magnetospheric flows during solar wind dynamic pressure pulse
Tian, Anmin; Shen, Xiaochen; Shi, Quanqi
Department空间科学部
Source Publication2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
2014
Language英语
ISBN9781467352253
AbstractThe response scenario of dayside magnetospheric plasma flows to the sudden increase of solar wind dynamic pressures was studied with 5 events from THEMIS observation. In all events we observed bipolar Vx(-/+) signatures as a response. The inferred flow vortices presented to be rotating clockwise and counterclockwise in the morning and afternoon side, respectively, as see from the north. Moreover, the pre and after noon flow vortices move toward -y and +y direction. The in situ observation of dayside plasmasheet flow vortices may provide a new possible mechanism for the solar wind dynamic impulse associated dayside ionospheric convection vortices.
Conference Name2014 31th URSI General Assembly and Scientific Symposium, URSI GASS 2014
Conference DateAugust 16, 2014 - August 23, 2014
Conference PlaceBeijing, China
Indexed ByEI
Document Type会议论文
Identifierhttp://ir.nssc.ac.cn/handle/122/4321
Collection空间科学部
Recommended Citation
GB/T 7714
Tian, Anmin,Shen, Xiaochen,Shi, Quanqi. Characteristics of dayside magnetospheric flows during solar wind dynamic pressure pulse[C]:Institute of Electrical and Electronics Engineers Inc.,2014.
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20146929930.pdf(832KB)会议论文 开放获取CC BY-NC-SAApplication Full Text
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