scholarly journals Electron acceleration by parallel and perpendicular electric fields during magnetic reconnection without guide field

2015 ◽  
Vol 120 (11) ◽  
pp. 9355-9367 ◽  
Author(s):  
N. Bessho ◽  
L.‐J. Chen ◽  
K. Germaschewski ◽  
A. Bhattacharjee
2015 ◽  
Vol 32 (9) ◽  
pp. 095202 ◽  
Author(s):  
Xiang-Sheng Lai ◽  
Meng Zhou ◽  
Xiao-Hua Deng ◽  
Tang-Mu Li ◽  
Shi-Yong Huang

2018 ◽  
Vol 36 (2) ◽  
pp. 373-379 ◽  
Author(s):  
Song Fu ◽  
Shiyong Huang ◽  
Meng Zhou ◽  
Binbin Ni ◽  
Xiaohua Deng

Abstract. It has been shown that the guide field substantially modifies the structure of the reconnection layer. For instance, the Hall magnetic and electric fields are distorted in guide field reconnection compared to reconnection without guide fields (i.e., anti-parallel reconnection). In this paper, we performed 2.5-D electromagnetic full particle simulation to study the electric field structures in magnetic reconnection under different initial guide fields (Bg). Once the amplitude of a guide field exceeds 0.3 times the asymptotic magnetic field B0, the traditional bipolar Hall electric field is clearly replaced by a tripolar electric field, which consists of a newly emerged electric field and the bipolar Hall electric field. The newly emerged electric field is a convective electric field about one ion inertial length away from the neutral sheet. It arises from the disappearance of the Hall electric field due to the substantial modification of the magnetic field and electric current by the imposed guide field. The peak magnitude of this new electric field increases linearly with the increment of guide field strength. Possible applications of these results to space observations are also discussed. Keywords. Space plasma physics (magnetic reconnection)


2000 ◽  
Vol 195 ◽  
pp. 311-312
Author(s):  
Y. E. Litvinenko

Fast magnetic reconnection in extragalactic jets leads to electron acceleration by the DC electric field in the reconnecting current sheet. The maximum electron energy (γ > 106) and the acceleration time (< 106 s) are determined by the magnetic field dynamics in the sheet.


2008 ◽  
Vol 15 (3) ◽  
pp. 032903 ◽  
Author(s):  
Weigang Wan ◽  
Giovanni Lapenta ◽  
Gian Luca Delzanno ◽  
Jan Egedal

2015 ◽  
Vol 22 (10) ◽  
pp. 100704 ◽  
Author(s):  
J. T. Dahlin ◽  
J. F. Drake ◽  
M. Swisdak

2017 ◽  
Vol 24 (5) ◽  
pp. 052113 ◽  
Author(s):  
Huanyu Wang ◽  
Quanming Lu ◽  
Can Huang ◽  
Shui Wang

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