Generalized lower-hybrid drift instabilities in current-sheet equilibrium

2002 ◽  
Vol 9 (5) ◽  
pp. 1526-1538 ◽  
Author(s):  
Peter H. Yoon ◽  
Anthony T. Y. Lui ◽  
Mikhail I. Sitnov
Keyword(s):  
2010 ◽  
Vol 17 (10) ◽  
pp. 102102 ◽  
Author(s):  
Dandan Zou ◽  
Weihong Yang ◽  
Yinhua Chen ◽  
P. H. Yoon

2009 ◽  
Vol 16 (4) ◽  
pp. 042107 ◽  
Author(s):  
Feng Huang ◽  
Yinhua Chen ◽  
Guifen Shi ◽  
Zuquan Hu ◽  
Haiou Peng ◽  
...  

2014 ◽  
Vol 21 (5) ◽  
pp. 052104 ◽  
Author(s):  
K. Tummel ◽  
L. Chen ◽  
Z. Wang ◽  
X. Y. Wang ◽  
Y. Lin

2013 ◽  
Vol 87 (6) ◽  
pp. 065501 ◽  
Author(s):  
Feng Huang ◽  
Guohong Liu ◽  
Yinhua Chen ◽  
M Y Yu ◽  
Fei Yan ◽  
...  

2002 ◽  
Author(s):  
T. A. Carter ◽  
M. Yamada ◽  
H. Ji ◽  
R. M. Kulsrud ◽  
F. Trintchouck

2021 ◽  
Vol 87 (1) ◽  
Author(s):  
F. Allmann-Rahn ◽  
S. Lautenbach ◽  
R. Grauer ◽  
R. D. Sydora

Fluid models that approximate kinetic effects have received attention recently in the modelling of large-scale plasmas such as planetary magnetospheres. In three-dimensional reconnection, both reconnection itself and current sheet instabilities need to be represented appropriately. We show that a heat flux closure based on pressure gradients enables a 10-moment fluid model to capture key properties of the lower-hybrid drift instability (LHDI) within a reconnection simulation. Characteristics of the instability are examined with kinetic and fluid continuum models, and its role in the three-dimensional reconnection simulation is analysed. The saturation level of the electromagnetic LHDI is higher than expected, which leads to strong kinking of the current sheet. Therefore, the magnitude of the initial perturbation has significant impact on the resulting turbulence.


2002 ◽  
Vol 9 (8) ◽  
pp. 3272-3288 ◽  
Author(s):  
T. A. Carter ◽  
M. Yamada ◽  
H. Ji ◽  
R. M. Kulsrud ◽  
F. Trintchouk

2008 ◽  
Vol 10 (4) ◽  
pp. 416-421
Author(s):  
Hu Youjun ◽  
Yang Weihong ◽  
Chen Yinhua ◽  
Huang Feng ◽  
Wang Feihu ◽  
...  

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