During the last few years, changes in the state of polarization of a class of random electromagnetic beams (so-called electromagnetic Gaussian Schell-model beams), propagating in free space have been investigated. In the present paper, we extend the analysis to propagation of such beams in homogeneous, isotropic, non-absorbing atmospheric turbulence. We find that the effects of turbulence on the state of polarization are most significant when the atmospheric fluctuations are weak or moderate, whereas in a strong regime of atmospheric fluctuations the state of polarization of the beam returns to its original state. Our results might find possible useful applications for sensing, imaging and communication through the atmosphere. © 2005 Taylor...
We show that the state of polarization of the polarized portion of a random, statistically stationar...
The general model of beam wander for a coherent Gaussian beam propagating through atmospheric turbul...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
During the last few years, changes in the state of polarization of a class of random electromagnetic...
During the last few years, changes in the state of polarization of a class of random electromagnetic...
We study the changes in the degree of polarization of an electromagnetic Gaussian Schell-model beam,...
We study the changes in the degree of polarization of an electromagnetic Gaussian Schell-model beam,...
Taking the random electromagnetic cosh-Gaussian beam as a typical example of random electromagnetic ...
In this paper, we study the effects of turbulent atmosphere on the degree of polarization of a parti...
It is shown analytically that the degree of polarization of a beam generated by an electromagnetic G...
It is shown analytically that the degree of polarization of a beam generated by an electromagnetic G...
We report analytic formulas for the elements of the e 2 X 2 cross-spectral density matrix of a stoch...
Based on extended Huygens-Fresnel principle, analytical expressions of beam width and far-field angu...
Polarization properties of electromagnetic Gaussian Schell-model beams propagating through the aniso...
We show that the state of polarization of the polarized portion of a random, statistically stationar...
We show that the state of polarization of the polarized portion of a random, statistically stationar...
The general model of beam wander for a coherent Gaussian beam propagating through atmospheric turbul...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...
During the last few years, changes in the state of polarization of a class of random electromagnetic...
During the last few years, changes in the state of polarization of a class of random electromagnetic...
We study the changes in the degree of polarization of an electromagnetic Gaussian Schell-model beam,...
We study the changes in the degree of polarization of an electromagnetic Gaussian Schell-model beam,...
Taking the random electromagnetic cosh-Gaussian beam as a typical example of random electromagnetic ...
In this paper, we study the effects of turbulent atmosphere on the degree of polarization of a parti...
It is shown analytically that the degree of polarization of a beam generated by an electromagnetic G...
It is shown analytically that the degree of polarization of a beam generated by an electromagnetic G...
We report analytic formulas for the elements of the e 2 X 2 cross-spectral density matrix of a stoch...
Based on extended Huygens-Fresnel principle, analytical expressions of beam width and far-field angu...
Polarization properties of electromagnetic Gaussian Schell-model beams propagating through the aniso...
We show that the state of polarization of the polarized portion of a random, statistically stationar...
We show that the state of polarization of the polarized portion of a random, statistically stationar...
The general model of beam wander for a coherent Gaussian beam propagating through atmospheric turbul...
It is known that the spectrum of light can change on propagation, even in free space. Such changes a...