Effects on electrostatic fields excited by radio-frequency waves in a bounded plasma due to the ponderomotive force

1992 ◽  
Vol 47 (2) ◽  
pp. 271-279
Author(s):  
C. R. Gutiérrez-Tapia

A one-dimensional model explaining the mechanism of excitation of electrostatic fields by linearly polarized radio-frequency waves in a plasma layer is presented. It is shown that the ponderomotive and driving forces influence this process strongly; however, these forces act at different times when a wave front passes through the plasma. We consider a semi-infinite plasma, and a plasma layer with and without current. It is observed that near to the plasma boundaries, where the electric field is large, there arise amplitude field oscillations, which are slowly exponentially damped in space. It is shown that the physical processes arising near the boundary x = L are similar to those at the boundary x = 0. It is seen that the current in the plasma block excitation at the boundary x = L.

2006 ◽  
Vol 19 (2) ◽  
pp. 209-217
Author(s):  
Iliycho Iliev ◽  
Snezhana Gocheva-Ilieva

Variety of electron, ion and plasma technologies as well as gas discharge devices operate in fixed form of the discharge. The transition from weak to heavy current in radio-frequency low-current discharge leads to instabilities in physical processes and it is very critical for the normal functionality of the technology or device. In this paper by means of Townsend criterion the influence of the incoming electric power and voltage on this transition in a cross-section of the discharge is numerically simulated. The calculations show a possible change of applied designed power up to 32% without weak to heavy-current transition. It is also obtained that the rise in 40% of the pressure can change the critical breakdown power only up to 12%. These results are in agreement with the simple analytical one-dimensional models and experimental data.


2021 ◽  
Vol 28 (8) ◽  
pp. 083501
Author(s):  
J. Moritz ◽  
S. Heuraux ◽  
E. Gravier ◽  
M. Lesur ◽  
F. Brochard ◽  
...  

2020 ◽  
Vol 175 (11-12) ◽  
pp. 976-980
Author(s):  
Abhay K. Ram ◽  
K. Hizanidis ◽  
F. Bairaktaris ◽  
A. Papadopoulos ◽  
S.-I. Valvis

2010 ◽  
Vol 17 (5) ◽  
pp. 467-479 ◽  
Author(s):  
B. T. Tsurutani ◽  
G. S. Lakhina ◽  
O. P. Verkhoglyadova ◽  
E. Echer ◽  
F. L. Guarnieri

Abstract. We discuss two different physical processes that create localized high β plasma regions. One is nonlinear wave-steepening, generating magnetic decreases (MDs) by a ponderomotive force. The other is the mirror instability generating alternating high and low β plasma regions. It is demonstrated that MDs and mirror modes are observationally quite different structures. MDs spatially occur in interplanetary space and mirror modes primarily in planetary magnetosheaths. MDs are characterized by: 1) variable (exponentially decreasing number with increasing) angular changes, 2) variable (exponentially decreasing) thicknesses, and 3) no characteristic inter-event spacings. In sharp contrast, mirror modes are characterized by: 1) little or no angular changes across the structures, 2) a characteristic scale size, and 3) are quasiperiodic in nature. Arguments are presented for the recently observed magnetic dips in the heliosheath being mirror mode structures. The sources of free energy for instability are discussed. Both structures are important for energetic particle transport in astrophysical and heliospheric plasmas.


2020 ◽  
Vol 175 (11-12) ◽  
pp. 1037-1041
Author(s):  
C. Standfield ◽  
T. Smith ◽  
I. Mombo ◽  
M. Rhinehart ◽  
P. Adegbaye ◽  
...  

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

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