A new model for the electron pressure nongyrotropy in the outer electron diffusion region

2016 ◽  
Vol 43 (20) ◽  
pp. 10,565-10,573 ◽  
Author(s):  
A. Divin ◽  
V. Semenov ◽  
D. Korovinskiy ◽  
S. Markidis ◽  
J. Deca ◽  
...  
2019 ◽  
Vol 26 (10) ◽  
pp. 102305
Author(s):  
A. Divin ◽  
V. Semenov ◽  
I. Zaitsev ◽  
D. Korovinskiy ◽  
J. Deca ◽  
...  

2010 ◽  
Vol 17 (12) ◽  
pp. 122102 ◽  
Author(s):  
A. Divin ◽  
S. Markidis ◽  
G. Lapenta ◽  
V. S. Semenov ◽  
N. V. Erkaev ◽  
...  

2017 ◽  
Vol 44 (5) ◽  
pp. 2049-2059 ◽  
Author(s):  
K.‐J. Hwang ◽  
D. G. Sibeck ◽  
E. Choi ◽  
L.‐J. Chen ◽  
R. E. Ergun ◽  
...  

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

2016 ◽  
Vol 121 (5) ◽  
pp. 4279-4290 ◽  
Author(s):  
B. U. Ö. Sonnerup ◽  
H. Hasegawa ◽  
R. E. Denton ◽  
T. K. M. Nakamura

2021 ◽  
Author(s):  
Takuma Nakamura ◽  
Hiroshi Hasegawa ◽  
Tai Phan ◽  
Kevin Genestreti ◽  
Richard Denton ◽  
...  

<p>Magnetic reconnection is a key fundamental process in collisionless plasmas that explosively converts magnetic energy to plasma kinetic and thermal energies through a change of magnetic field topology in an electron-scale central region called the electron diffusion region. Past simulations and observations demonstrated that this process causes efficient energy conversion through the formation of multiple macro-scale or micro-scale magnetic islands/flux ropes. However, how these different spatiotemporal scale phenomena are coupled is still poorly understood. In this study, to investigate the turbulent evolution of magnetic reconnection, we perform a new large-scale fully kinetic simulation of a thin current sheet considering a power-law spectrum of initial fluctuations in the magnetic field as frequently observed in the Earth’s magnetotail. The simulation demonstrates that during a macro-scale evolution of turbulent reconnection, the merging of macro-scale islands results in reduction of the rate of reconnection as well as the aspect ratio of the electron diffusion region. This allows the repeated, quick formation of new electron-scale islands within the electron diffusion region, leading to an efficient energy cascade between macro- and micro-scales. The simulation also demonstrates that a strong electron acceleration/heating occurs during the micro-scale island evolution within the EDR. These new findings indicate the importance of non-steady features of the EDR to comprehensively understand the energy conversion and cascade processes in collisionless reconnection.</p>


2019 ◽  
Vol 124 (12) ◽  
pp. 10153-10169
Author(s):  
S. Hoilijoki ◽  
R. E. Ergun ◽  
S. J. Schwartz ◽  
S. Eriksson ◽  
F. D. Wilder ◽  
...  

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