The evolution of the ion diffusion region during collisionless magnetic reconnection in a force-free current sheet

2015 ◽  
Vol 22 (9) ◽  
pp. 092110 ◽  
Author(s):  
Fushun Zhou ◽  
Can Huang ◽  
Quanming Lu ◽  
Jinlin Xie ◽  
Shui Wang
2015 ◽  
Vol 120 (5) ◽  
pp. 3535-3551 ◽  
Author(s):  
Y. H. Liu ◽  
C. G. Mouikis ◽  
L. M. Kistler ◽  
S. Wang ◽  
V. Roytershteyn ◽  
...  

2012 ◽  
Vol 30 (1) ◽  
pp. 109-117 ◽  
Author(s):  
A. L. Borg ◽  
M. G. G. T. Taylor ◽  
J. P. Eastwood

Abstract. The Earth's magnetosphere provides an excellent laboratory for magnetic reconnection research. In particular, the magnetotail current sheet that is formed between the interface of the similar Northern and Southern Hemispheres of the magnetotail provides a relatively stable symmetric reconnection configuration that can be used to study basic aspects of the reconnection process. Of particular importance is the manner in which electrons are processed by the reconnection. Simulations and satellite data analyses of the ion diffusion region have suggested that the fluxes of electrons in the inflow regions of reconnection are greater in the directions parallel and anti-parallel to the magnetic field (field-aligned) whereas the electron flux in the outflow region is distributed more isotropically. However, this has only been studied experimentally on a case-by-case basis. In this paper, we investigate this claim by analyzing the degree of bulk electron field alignment in the outflow and inflow regions during encounters of the magnetic reconnection ion diffusion region by the Cluster spacecraft in the years 2001–2006. We demonstrate that while the median electron flux in the inflow region is indeed more field aligned than in the outflow region during some ion diffusion region encounters, the variation of the signature across events is so large that it cannot be said to be a general feature of magnetic reconnection in the Earth's magnetotail.


2011 ◽  
Vol 18 (11) ◽  
pp. 111204 ◽  
Author(s):  
P. Wu ◽  
M. A. Shay ◽  
T. D. Phan ◽  
M. Oieroset ◽  
M. Oka

2015 ◽  
Vol 12 (3) ◽  
pp. 263-267 ◽  
Author(s):  
Rongsheng Wang ◽  
Quanming Lu ◽  
Rumi Nakamura ◽  
Can Huang ◽  
Aimin Du ◽  
...  

2021 ◽  
Vol 922 (1) ◽  
pp. 54
Author(s):  
S. Y. Huang ◽  
Q. Y. Xiong ◽  
L. F. Song ◽  
J. Nan ◽  
Z. G. Yuan ◽  
...  

Abstract In the standard model of magnetic reconnection, both ions and electrons couple to the newly reconnected magnetic field lines and are ejected away from the reconnection diffusion region in the form of bidirectional burst ion/electron jets. Recent observations propose a new model: electron-only magnetic reconnection without ion coupling in an electron-scale current sheet. Based on the data from the Magnetospheric Multiscale (MMS) mission, we observe a long-extension inner electron diffusion region (EDR) at least 40 d i away from the X-line at the Earth’s magnetopause, implying that the extension of EDR is much longer than the prediction of the theory and simulations. This inner EDR is embedded in an ion-scale current sheet (the width of ∼4 d i, d i is ion inertial length). However, such ongoing magnetic reconnection was not accompanied with burst ion outflow, implying the presence of electron-only reconnection in an ion-scale current sheet. Our observations present a new challenge for understanding the model of standard magnetic reconnection and the electron-only reconnection model in an electron-scale current sheet.


2008 ◽  
Vol 101 (8) ◽  
Author(s):  
Yang Ren ◽  
Masaaki Yamada ◽  
Hantao Ji ◽  
Stefan P. Gerhardt ◽  
Russell Kulsrud

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