Theory and simulation of lower-hybrid drift instability for current sheet with guide field

2008 ◽  
Vol 15 (11) ◽  
pp. 112103 ◽  
Author(s):  
P. H. Yoon ◽  
Y. Lin ◽  
X. Y. Wang ◽  
A. T. Y. Lui
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 ◽  
...  

2020 ◽  
Author(s):  
Binbin Tang ◽  
Wenya Li ◽  
Daniel Graham ◽  
Chi Wang ◽  
Yuri Khotyaintsev ◽  
...  

<div>Lower hybrid waves are investigated at the magnetosheath separatrix region in asymmetric guide-field reconnection at Earth’s magnetopause by using MMS observations. These waves are found in a limited region, depending on the density gradient across the separatrix, and they are driven by the lower hybrid drift instability. Properties of these waves are presented: (1) the waves propagate towards the x-line due to the out-of-plane magnetic field, consistent with the electron drift direction; (2) the wave potential is about 20% of the electron temperature. These drift waves effectively produce cross-field particle diffusion, enabling the entry of magnetosheath electrons into the exhaust region.</div>


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.


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

2021 ◽  
Author(s):  
Florian Allmann-Rahn ◽  
Simon Lautenbach ◽  
Richard Sydora ◽  
Rainer Grauer

<p>The electromagnetic branch of the lower-hybrid drift instability (LHDI) can lead to kinking of current sheets and fluctuations in the magnetic field and is present for example in Earth’s magnetosphere. Previous particle-in-cell studies suggested that the electromagnetic LHDI’s saturation is at a moderate level and that strong current sheet kinking is only caused by slower kink-type modes. Here, we present kinetic continuum simulations that show strong kinking and high saturation levels of the B-field fluctuations. Has the impact of the electromagnetic LHDI been underestimated? The capability of the LHDI to produce x-lines and turbulence in 3D reconnection is discussed at the example of ten-moment multi-fluid simulations.</p>


2008 ◽  
Vol 25 (7) ◽  
pp. 2725-2728 ◽  
Author(s):  
Guo Fan ◽  
Lu Quan-Ming ◽  
Guo Jun ◽  
Wang Shui

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