Transverse mode analysis of a laser beam with a non-optical technique

2008 ◽  
Author(s):  
R. de Saint Denis ◽  
M. Fromager ◽  
F. Porée ◽  
K. Ait-Ameur
1995 ◽  
Vol 34 (34) ◽  
pp. 7974 ◽  
Author(s):  
Antonello Cutolo ◽  
Tommaso Isernia ◽  
IIdegonda Izzo ◽  
Rocco Pierri ◽  
Luigi Zeni

2001 ◽  
Vol 2001.50 (0) ◽  
pp. 39-40
Author(s):  
Toshihiro Kobayashi ◽  
Jun Ohsawa ◽  
Naohiro Yamaguchi ◽  
Tamio Hara

2010 ◽  
Vol 39 (11) ◽  
pp. 2040-2044
Author(s):  
周娜 ZHOU Na ◽  
王石语 WANG Shiyu ◽  
过振 GUO Zhen ◽  
蔡德芳 CAI Defang ◽  
文建国 WEN Jianguo ◽  
...  

1985 ◽  
Vol 40 (8) ◽  
pp. 826-833
Author(s):  
Rajkamal Sanghvi ◽  
R. K. Chhajlani

The Rayleigh-Taylor (RT) instability of a stratified and viscid magnetoplasma including the effects of "finite-resistivity and suspended particles is investigated using normal mode analysis. The horizontal magnetic field and the viscosity of the medium are assumed to be variable. The dispersion relation, which is obtained for the general case on employing boundary conditions appropriate to the case of two free boundaries, is then specialized for the longitudinal and transverse modes. It is found that the criterion of stable stratification remains essentially unchanged and that the unstable stratification for the longitudinal mode can be stabilized for a certain wave number band, whereas the transverse mode remains unstable or all wave numbers which can be stabilized by a suitable choice of the magnetic field for vanishing resistivity. Thus, resistivity is found to have a destabilizing influence on the RT configuration. The growth rates of the unstable RT modes with the kinematic viscosity and the relaxation frequency parameter of the suspended particles have been analytically evaluated. Dust (suspended particles) tends to stabilize the configuration when the medium is considered viscid with infinite conductivity. The kinematic viscosity has a stabilizing influence on the ideal plasma modes.


2014 ◽  
Vol 81 (2) ◽  
Author(s):  
Prerana Sharma ◽  
R. K. Chhajlani

The Jeans self-gravitational instability is studied for dense quantum viscous plasma with Hall term and intrinsic magnetization generated by collective electron spin. The quantum magnetohydrodynamic model is employed to formulate the basic equations of the problem. The dispersion relation is obtained using the normal mode analysis, and further reduced for both transverse and longitudinal modes of propagation. The transverse mode of propagation is found to be unaffected by the Hall term but affected by quantum effect, viscosity, and magnetization parameters. The Jeans criterion of instability in the transverse direction is modified by Alfven velocity, magnetization parameter, and quantum effect. The non-gravitating magnetized mode is obtained in the longitudinal direction, which is modified by Hall parameter and is not affected by quantum term, whereas the gravitational mode is unaffected by the magnetization parameter but affected by viscosity and quantum parameters. It is observed that the Jeans condition of instability is affected by the quantum term. The growth rate of Jeans instability is plotted for various values of magnetization, quantum, and viscosity parameters of the quantum plasma medium.


2020 ◽  
Vol 12 (4) ◽  
pp. 1-6
Author(s):  
Yinli Zhou ◽  
Xing Zhang ◽  
Jianwei Zhang ◽  
Youwen Huang ◽  
Yugang Zeng ◽  
...  

2011 ◽  
Vol 38 (1) ◽  
pp. 0108004
Author(s):  
周娜 Zhou Na ◽  
王石语 Wang Shiyu ◽  
过振 Guo Zhen ◽  
蔡德芳 Cai Defang ◽  
文建国 Wen Jianguo ◽  
...  

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