Magnetic reconnection and cold plasma at the magnetopause

被引:32
|
作者
Andre, M. [1 ]
Vaivads, A. [1 ]
Khotyaintsev, Y. V. [1 ]
Laitinen, T. [1 ]
Nilsson, H. [3 ]
Stenberg, G. [3 ]
Fazakerley, A. [2 ]
Trotignon, J. G. [4 ]
机构
[1] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
[2] Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
[3] Swedish Inst Space Phys, SE-98128 Kiruna, Sweden
[4] Univ Orleans, Lab Phys & Chim Environm & Espace, F-45071 Orleans 2, France
关键词
DENSITY;
D O I
10.1029/2010GL044611
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
We report on detailed observations by the four Cluster spacecraft of magnetic reconnection and a Flux Transfer Event (FTE) at the magnetopause. We detect cold (eV) plasma at the magnetopause with two independent methods. We show that the cold ions can be essential for the electric field normal to the current sheet in the separatrix region at the edge of the FTE and for the associated acceleration of ions from the magnetosphere into the reconnection jet. The cold ions have small enough gyroradii to drift inside the limited separatrix region and the normal electric field can be balanced by this drift, E approximate to -v x B. The separatrix region also includes cold accelerated electrons, as part of the reconnection current circuit. Citation: Andre, M., A. Vaivads, Y. V. Khotyaintsev, T. Laitinen, H. Nilsson, G. Stenberg, A. Fazakerley, and J. G. Trotignon (2010), Magnetic reconnection and cold plasma at the magnetopause, Geophys. Res. Lett., 37, L22108, doi:10.1029/2010GL044611.
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页数:5
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