共 15 条
On the electron diffusion region in asymmetric reconnection with a guide magnetic field
被引:49
作者:
Hesse, Michael
[1
]
Liu, Yi-Hsin
[1
]
Chen, Li-Jen
[1
]
Bessho, Naoki
[1
]
Kuznetsova, Masha
[1
]
Birn, Joachim
[2
,3
]
Burch, James L.
[4
]
机构:
[1] NASA, Goddard Space Flight Ctr, Heliophys Sci Div, Greenbelt, MD USA
[2] Space Sci Inst, Boulder, CO USA
[3] Los Alamos Natl Lab, Los Alamos, NM USA
[4] SW Res Inst, San Antonio, TX USA
基金:
美国国家科学基金会;
关键词:
magnetic reconnection;
magnetopause;
magnetospheric multiscale;
kinetic physics;
distribution function;
plasma physics;
D O I:
10.1002/2016GL068373
中图分类号:
P [天文学、地球科学];
学科分类号:
07 ;
摘要:
Particle-in-cell simulations in a 2.5-D geometry and analytical theory are employed to study the electron diffusion region in asymmetric reconnection with a guide magnetic field. The analysis presented here demonstrates that similar to the case without guide field, in-plane flow stagnation and null of the in-plane magnetic field are well separated. In addition, it is shown that the electric field at the local magnetic X point is again dominated by inertial effects, whereas it remains dominated by nongyrotropic pressure effects at the in-plane flow stagnation point. A comparison between local electron Larmor radii and the magnetic gradient scale lengths predicts that distribution should become nongyrotropic in a region enveloping both field reversal and flow stagnation points. This prediction is verified by an analysis of modeled electron distributions, which show clear evidence of mixing in the critical region.
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页码:2359 / 2364
页数:6
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