Rotation of dust particles in an inhomogeneous weak magnetic field in a DC glow discharge

2021 ◽  
Vol 28 (7) ◽  
pp. 074503
Author(s):  
A. R. Abdirakhmanov ◽  
N. Kh. Bastykova ◽  
S. K. Kodanova ◽  
T. S. Ramazanov
2017 ◽  
Vol 2017 ◽  
pp. 1-8 ◽  
Author(s):  
Shen Gao ◽  
Shixiu Chen ◽  
Zengchao Ji ◽  
Wei Tian ◽  
Jun Chen

On the basis of fluid approximation, an improved version of the model for the description of dc glow discharge plasma in the axial magnetic field was successfully developed. The model has yielded a set of analytic formulas for the physical quantities concerned from the electron and ion fluids equations and Poisson equation. The calculated results satisfy the practical boundary conditions. Results obtained from the model reveal that although the differential equations under the condition of axial magnetic field are consistent with the differential equations without considering the magnetic field, the solution of the equations is not completely consistent. The results show that the stronger the magnetic field, the greater the plasma density.


2018 ◽  
Vol 123 (10) ◽  
pp. 103301 ◽  
Author(s):  
Ruihuan Tian ◽  
Chengxun Yuan ◽  
Hui Li ◽  
Yonggan Liang ◽  
Jian Wu ◽  
...  

2019 ◽  
Vol 28 (8) ◽  
pp. 085020 ◽  
Author(s):  
E S Dzlieva ◽  
L G D’yachkov ◽  
L A Novikov ◽  
S I Pavlov ◽  
V Yu Karasev

2018 ◽  
Vol 25 (2) ◽  
pp. 023701 ◽  
Author(s):  
Yonggan Liang ◽  
Chengxun Yuan ◽  
Hui Li ◽  
Ruihuan Tian ◽  
Jian Wu ◽  
...  

Molecules ◽  
2021 ◽  
Vol 26 (13) ◽  
pp. 3788
Author(s):  
Elena S. Dzlieva ◽  
Lev G. D’yachkov ◽  
Leontiy A. Novikov ◽  
Sergey I. Pavlov ◽  
Viktor Y. Karasev

We study the dynamics of dust particles in a stratified glow discharge in inhomogeneous magnetic fields. Dust structures are formed in standing striations, in which traps for dust particles arise. When a magnetic field is applied, these structures begin to rotate. The observations were carried out in striations near the end of the solenoid, where the region of an inhomogeneous magnetic field begins. With an increase in the magnetic field, the dusty structure can be deformed. The rotation of a dusty structure in an inhomogeneous magnetic field has been studied in detail; it has its own peculiarities in comparison with rotation in a uniform field. We have considered the mechanisms of such rotation and estimated its velocity.


2019 ◽  
Vol 47 (7) ◽  
pp. 3036-3040 ◽  
Author(s):  
A. R. Abdirakhmanov ◽  
Zh. A. Moldabekov ◽  
S. K. Kodanova ◽  
M. K. Dosbolayev ◽  
T. S. Ramazanov

2005 ◽  
pp. 465-476
Author(s):  
V.E. Fortov ◽  
A.G. Khrapak ◽  
V.I. Molotkov ◽  
O.F. Petrov ◽  
M.Y. Poustylnik ◽  
...  

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