scholarly journals Experimental Study of Magnetic Reconnection in Partially Ionized Plasmas Using Rotating Magnetic Field

2019 ◽  
Vol 14 (0) ◽  
pp. 3401054-3401054 ◽  
Author(s):  
Yoshifumi TAKAHATA ◽  
Ryoma YANAI ◽  
Michiaki INOMOTO
1965 ◽  
Vol 18 (4) ◽  
pp. 309 ◽  
Author(s):  
HA Blevin ◽  
RB Miller

The electron density distribution in a linear pinch discharge with a transverse rotating magnetic field is calculated for partially ionized plasmas. Numerical examples are given for distributions in the plasma with and without externally applied axial magnetic fields, and with different degrees of ionization.


2019 ◽  
Vol 122 (1) ◽  
Author(s):  
J. Jara-Almonte ◽  
H. Ji ◽  
J. Yoo ◽  
M. Yamada ◽  
W. Fox ◽  
...  

1977 ◽  
Vol 18 (1) ◽  
pp. 77-89 ◽  
Author(s):  
L. Bighel ◽  
A. R. Collins ◽  
N. F. Cramer

The structure of MHD switch-on shocks propagating along a magnetic field into an upstream partially ionized plasma is studied experimentally and theoretically. Detailed measurements of density, temperature and magnetic field are presented, and compared with a model based on the fluid equations for electrons, ions and neutral atoms. The main feature of the model is that dissipation of shock energy occurs primarily through ion collisions with neutrals. According to the model, at low upstreain ionization levels, ions and neutrals are preferentially heated above the electrons. At high ionization levels, the electrons are more strongly heated. This is found to be in agreement with the shock structures obtained for 4 switch-on shocks, differing in the level of upstream ionization.


Author(s):  
Lei Ni ◽  
Hantao Ji ◽  
Nicholas A. Murphy ◽  
Jonathan Jara-Almonte

Magnetic reconnection has been intensively studied in fully ionized plasmas. However, plasmas are often partially ionized in astrophysical environments. The interactions between the neutral particles and ionized plasmas might strongly affect the reconnection mechanisms. We review magnetic reconnection in partially ionized plasmas in different environments from theoretical, numerical, observational and experimental points of view. We focus on mechanisms which make magnetic reconnection fast enough to compare with observations, especially on the reconnection events in the low solar atmosphere. The heating mechanisms and the related observational evidence of the reconnection process in the partially ionized low solar atmosphere are also discussed. We describe magnetic reconnection in weakly ionized astrophysical environments, including the interstellar medium and protostellar discs. We present recent achievements about fast reconnection in laboratory experiments for partially ionized plasmas.


2011 ◽  
Vol 18 (11) ◽  
pp. 111211 ◽  
Author(s):  
Ellen G. Zweibel ◽  
Eric Lawrence ◽  
Jongsoo Yoo ◽  
Hantao Ji ◽  
Masaaki Yamada ◽  
...  

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