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.
引用
收藏
页码:2359 / 2364
页数:6
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