Electromagnetic Hanbury Brown and Twiss Effect in Atmospheric Turbulence
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The evolution of the 4 × 4 matrix with elements being the scintillation indices of the single-point Stokes parameters of a stationary electromagnetic beam-like optical field in classic, weak atmospheric turbulence is revealed. It is shown that depending on the choice of the source parameters, the source-induced changes in the matrix elements of the propagating beam and those produced by turbulence can be either range-separated or conjoined. For theoretical analysis, the unified theory of coherence and polarization is used together with the extended Huygens-Fresnel integral approach. The results can be of interest for building robust communication and sensing systems operating in the presence of atmospheric fluctuations.
1975 ◽
Vol 97
(2)
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pp. 581-594
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1984 ◽
Vol 99
(1-2)
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pp. 173-184
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1969 ◽
Vol 27
(4)
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pp. 319-336
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2020 ◽
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1977 ◽
Vol 66
(7)
◽
pp. 2806-2813
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