Influences of sub-Alfvénic shear flows on nonlinear evolution of magnetic reconnection in compressible plasmas

2011 ◽  
Vol 18 (9) ◽  
pp. 092112 ◽  
2011 ◽  
Vol 64 (2-3) ◽  
pp. 365-368 ◽  
Author(s):  
X. X. Li ◽  
X. Q. Lu ◽  
X. Y. Gong ◽  
Q. H. Huang

2012 ◽  
Vol 40 (5) ◽  
pp. 1416-1420
Author(s):  
Xin Xia Li ◽  
Xue Yu Gong ◽  
Xing Qing Lu

2015 ◽  
Vol 22 (5) ◽  
pp. 052110 ◽  
Author(s):  
Lin Wang ◽  
Xiao-Gang Wang ◽  
Xian-Qu Wang ◽  
Yue Liu

2008 ◽  
Vol 15 (8) ◽  
pp. 082109 ◽  
Author(s):  
Zheng-Xiong Wang ◽  
Xiaogang Wang ◽  
J. Q. Dong ◽  
Y. Kishimoto ◽  
J. Q. Li

2020 ◽  
Author(s):  
Susanne Flø Spinnangr ◽  
Paul Tenfjord ◽  
Michael Hesse ◽  
Cecilia Norgren ◽  
Norah Kwagala

<p>Our group has done extensive research on the fluid and kinetic effect of cold ion populations on the reconnection process, in an effort to identify factors that can lead to the onset or stopping of magnetic reconnection. Recent fully kinetic studies involving cold protons or oxygen have shown that flows of cold particles significantly modify the reconnection process, and that the nature of this modification is dependent on the configuration of these flows and the constituent ions of the flows. In this study we want to investigate how the reconnection process is affected by a shear flow of cold protons outside of the current sheet, using a 2.5D Particle-In-Cell simulation. The effect of shear flows on magnetic reconnection has investigated earlier, indicating a signifficant modification of the reconnection process. However, it is not clear how these effects will be influenced by the additional scale lengths introduced into the system by a cold ion flow. In particular we want to investigate how the current sheet and diffusion regions are altered by a cold shear flow on a kinetic level, and how the reconnection process is altered on ion scales and beyond. Preliminary results indicate that the shear flow introduces a tilt of the current sheet, which appears to be consistent with earlier studies. Results will be compared to our group’s earlier results involving symmetric and asymmetric flows of cold particles in the inflow regions, as well as existing simulations and observations of magnetic reconnection including warm shear flows.</p>


2019 ◽  
Vol 15 (S354) ◽  
pp. 189-194
Author(s):  
J. B. Climent ◽  
J. C. Guirado ◽  
R. Azulay ◽  
J. M. Marcaide

AbstractWe report the results of three VLBI observations of the pre-main-sequence star AB Doradus A at 8.4 GHz. With almost three years between consecutive observations, we found a complex structure at the expected position of this star for all epochs. Maps at epochs 2007 and 2010 show a double core-halo morphology while the 2013 map reveals three emission peaks with separations between 5 and 18 stellar radii. Furthermore, all maps show a clear variation of the source structure within the observing time. We consider a number of hypothesis in order to explain such observations, mainly: magnetic reconnection in loops on the polar cap, a more general loop scenario and a close companion to AB Dor A.


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