Space‐charge wave propagation in inhomogeneous waveguides

1985 ◽  
Vol 28 (1) ◽  
pp. 358-365 ◽  
Author(s):  
A. Anselmo ◽  
G. Kerslick ◽  
J. A. Nation ◽  
G. Providakes
Keyword(s):  
Wave Propagation ◽  
Space Charge ◽  
Charge Wave ◽  
Space Charge Wave

Nonlinear space-charge wave propagation on thin annular electron beams

1984 ◽  
Vol 27 (7) ◽  
pp. 1808 ◽  
Author(s):  
D. L. Fenstermacher ◽  
C. E. Seyler
Keyword(s):  
Wave Propagation ◽  
Space Charge ◽  
Electron Beams ◽  
Charge Wave ◽  
Space Charge Wave

Space‐charge wave propagation on rippled electron beams

1976 ◽  
Vol 47 (10) ◽  
pp. 4464-4466 ◽  
Author(s):  
R. A. Mahaffey ◽  
D. B. Batchelor ◽  
A. W. Trivelpiece
Keyword(s):  
Wave Propagation ◽  
Space Charge ◽  
Electron Beams ◽  
Charge Wave ◽  
Space Charge Wave

scholarly journals Reactive medium instability of the space charge wave of ion beam in a plasma

1977 ◽  
Vol 64 (1) ◽  
pp. 53-55 ◽  
Author(s):  
Toshitaka Idehara ◽  
Kuni Nakajima ◽  
Yoshio Ishida
Keyword(s):  
Space Charge ◽  
Ion Beam ◽  
Reactive Medium ◽  
Charge Wave ◽  
Space Charge Wave

Resonant flow instability of space-charge waves in self-gravitating Lorentzian dusty plasma columns

2019 ◽  
Vol 97 (6) ◽  
pp. 651-655
Author(s):  
Myoung-Jae Lee ◽  
Young-Dae Jung
Keyword(s):  
Growth Rate ◽  
Space Charge ◽  
Dusty Plasma ◽  
Plasma Column ◽  
Flow Instability ◽  
Mode Analysis ◽  
Instability Mode ◽  
Resonant Instability ◽  
Charge Wave ◽  
Space Charge Wave

The dispersion characteristics and the resonant instability mode of the space-charge wave are investigated in a streaming Lorentzian dusty plasma column by using the normal mode analysis. The result shows that the non-thermal character of the Lorentzian cylindrical dusty plasma enhances the unstable property of the space-charge wave due to the beam–plasma interaction. It is found that the resonant growth rates of the space-charge wave increase with an increase of the harmonic-order of the root of the Bessel function. It is also found that the influence of the self-gravitation enhances the resonant growth rate of the space-charge wave of the Lorentzian cylindrical dusty plasma. In addition, it is found the resonant growth rate decreases with an increase of the radius of the dusty plasma column. The variation of the resonant instability mode due to the non-thermal character and geometric effects is also discussed.

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