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- W4313398876 endingPage "170487" @default.
- W4313398876 startingPage "170487" @default.
- W4313398876 abstract "A new beam called radially polarized Hermite-cos-Gaussian correlated Schell-model (RPHCGSM) beam is proposed. The propagation formulae of an RPHcGSM beam in oceanic turbulence are derived, and the propagation properties of such beam are analyzed. The results show that the spectral density distribution of an RPHcGSM beam in free space can be modulated by γ as distance increases; the beamlets will overlap when an RPHcGSM beam propagating through oceanic turbulence, and the stronger oceanic turbulence can accelerate the speed of beamlets evolving into Gauss beam. Moreover, the degree of polarization can become regular distribution and degree of coherence can become Gaussian distribution due to the influence of oceanic turbulence." @default.
- W4313398876 created "2023-01-06" @default.
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- W4313398876 date "2023-02-01" @default.
- W4313398876 modified "2023-10-16" @default.
- W4313398876 title "Propagation of a radially polarized Hermite-cos-Gaussian correlated Schell-model beam in oceanic turbulence" @default.
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- W4313398876 doi "https://doi.org/10.1016/j.ijleo.2022.170487" @default.
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