A One-Dimensional Particle-in-Cell Model of Plasma Build-Up in Vacuum Arcs

2011 ◽  
Vol 51 (1) ◽  
pp. 5-21 ◽  
Author(s):  
H. Timko ◽  
K. Matyash ◽  
R. Schneider ◽  
F. Djurabekova ◽  
K. Nordlund ◽  
...  
2017 ◽  
Vol 24 (10) ◽  
pp. 103511 ◽  
Author(s):  
Shenli Jia ◽  
Yongpeng Mo ◽  
Zongqian Shi ◽  
Junliang Li ◽  
Lijun Wang

2021 ◽  
Vol 28 (12) ◽  
pp. 123507
Author(s):  
T. Gyergyek ◽  
S. Costea ◽  
K. Bajt ◽  
A. Valič ◽  
J. Kovačič

2021 ◽  
Author(s):  
Jan Benáček ◽  
Marian Karlický

<p>We study how hot plasma that is released during a solar flare can be confined in its source and interact with surrounding colder plasma. The X-ray emission of coronal flare sources is well explained using Kappa velocity distribution. Therefore, we compare the difference in the confinement of plasma with Kappa and Maxwellian distribution. We use a 3D Particle-in-Cell code, which is large along magnetic field lines, effectively one-dimensional, but contains all electromagnetic effects. In the case with Kappa distribution, contrary to Maxwellian distribution, we found formation of several thermal fronts associated with double-layers that suppress particle fluxes. As the Kappa distribution of electrons forms an extended tail, more electrons are not confined by the first front and cause formation of multiple fronts. A beam of electrons from the hot part is formed at each front; it generates return current, Langmuir wave density depressions, and a double layer with a higher potential step than in the Maxwellian case. We compare the Kappa and Maxwellian cases and discuss how these processes could be observed.</p>


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