Kelvin-Helmholtz vortices and double mid-latitude reconnection at the Earth's magnetopause: Comparison between observations and simulations

被引:27
作者
Faganello, M. [1 ]
Califano, F. [2 ]
Pegoraro, F. [2 ]
Retino, A. [3 ]
机构
[1] Aix Marseille Univ, UMR CNRS 7345, Int Inst Fus Sci PIIM, Marseille, France
[2] Univ Pisa, Dept Phys, I-56100 Pisa, Italy
[3] Univ Paris 11, UPMC, Ecole Polytech, LPP,CNRS, Palaiseau, France
关键词
SOLAR-WIND; MAGNETIC RECONNECTION; INSTABILITY; INTERPLANETARY; MAGNETOSPHERE; MAGNETOTAIL; TRANSPORT; BOUNDARY; WAVES; LAYER;
D O I
10.1209/0295-5075/107/19001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Observational signatures of Kelvin-Helmholtz (K-H) vortices and of double mid-latitude reconnection are highlighted in satellite data of the THEMIS mission. It is shown that the plasma fluid quantities at the low-latitude flank of the Earth's magnetosphere are compatible with K-H vortices, as described by three-dimensional simulations. At the same time it is shown that the particle fluxes are compatible with the presence of magnetic-field lines, embedded in the K-H vortices, that close on Earth but are connected to the solar wind at low latitude. These field lines are generated during the K-H evolution by magnetic reconnection proceeding spontaneously in both hemispheres at mid-latitudes, allowing the solar-wind plasma to enter the Earth's magnetosphere directly. Copyright (C) EPLA, 2014
引用
收藏
页数:6
相关论文
共 36 条