scholarly journals Focusing of dark hollow Gaussian electromagnetic beams in a plasma

2009 ◽  
Vol 27 (1) ◽  
pp. 57-68 ◽  
Author(s):  
M.S. Sodha ◽  
S.K. Mishra ◽  
S. Misra

AbstractThis paper presents an investigation of the focusing of dark hollow Gaussian electromagnetic beams (HGB) in plasma, considering collisional, ponderomotive, and relativistic nonlinearities. A paraxial like approach, in which the parameters are expanded, in terms of radial distance from the maximum of irradiance rather than that from the axis, has been adopted. To highlight the nature of focusing, both critical curves and the divider curves have been obtained as a plot of dimensionless radius vs. power of the beam. The effect of the order of HGB (n), and nature of nonlinearity on self focusing of the beam has also been explored.

2009 ◽  
Vol 75 (6) ◽  
pp. 731-748 ◽  
Author(s):  
MAHENDRA SINGH SODHA ◽  
S. K. MISHRA ◽  
SHIKHA MISRA

AbstractThis paper presents an analysis and subsequent discussion of the self focusing of a dark hollow Gaussian electromagnetic beam (HGB) in a magnetoplasma, considering ponderomotive and collisional nonlinearities. A paraxial-like approach, in which the relevant parameters are expanded in terms of radial distance from the maximum of the irradiance rather than that from the axis, has been adopted to analyze the propagation of the HGB. The nature of self focusing is highlighted through the critical curves as a plot of dimensionless radius versus power of the beam. The effect of the magnetic field and the nature of the nonlinearity on self focusing of various order HGBs has also been explored.


1975 ◽  
Vol 46 (1) ◽  
pp. 369-372 ◽  
Author(s):  
D. P. Tewari ◽  
Awdhesh Kumar

2011 ◽  
Vol 77 (6) ◽  
pp. 777-784 ◽  
Author(s):  
RUCHIKA GUPTA ◽  
M. RAFAT ◽  
R. P. SHARMA

AbstractA paraxial-like approach has been invoked to understand the nature of propagation of a hollow Gaussian beam (HGB) propagating in plasma under the influence of relativistic non-linearity. In this approach, the parameters are expanded in terms of the radial distance from the maximum of irradiance rather than that from the axis. This paper investigates the excitation of plasma wave in a hot collision less plasma by HGB. On account of the × force, a plasma wave at 2ω0 (here, ω0 is the pump laser frequency) is generated. The solution of the HGB has been obtained within the paraxial ray approximation. Filamentary structures of the laser beam are observed due to relativistic non-linearity.


1974 ◽  
Vol 7 (16) ◽  
pp. 2188-2197 ◽  
Author(s):  
M S Sodha ◽  
R K Khanna ◽  
V K Tripathi

2004 ◽  
Vol 11 (9) ◽  
pp. 4275-4279 ◽  
Author(s):  
Ashutosh Sharma ◽  
M. P. Verma ◽  
M. S. Sodha

2008 ◽  
Vol 74 (4) ◽  
pp. 473-491 ◽  
Author(s):  
MAHENDRA SINGH SODHA ◽  
ASHUTOSH SHARMA

AbstractIn this paper the focusing/defocusing of (i) a single Gaussian electromagnetic beam and (ii) a number of coaxial Gaussian electromagnetic beams, propagating in the extraordinary mode along the Earth's magnetic field in the ionosphere has been investigated in the paraxial approximation. The growth of a sinusoidal instability on account of self-focusing has also been studied. The nonlinearity in the dielectric function, responsible for the focusing/defocusing arises from the redistribution of the electron density, caused by the non-uniform distribution of the electron temperature. The electron temperature is determined by the energy balance for electrons/ions taking into account the Ohmic heating, the collisions and the radiation from the sun. The wave frequency has been assumed to be greater than the plasma frequency. The electron cyclotron frequency due to the Earth's magnetic field in the ionosphere is much larger than the electron collision frequency. This is specifically true for a height of 150 km. Numerical results have been presented for a range of parameters and a discussion of the same has been presented.


1973 ◽  
Vol 2 (1) ◽  
pp. 39-42 ◽  
Author(s):  
M. S. Sodha ◽  
R. K. Khanna ◽  
V. K. Tripathi

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