Research on characteristics of radially polarized Lorentz correlated beam in anisotropic turbulent ocean

Abstract The cross-spectral density (CSD) matrix of radially polarized Lorentz correlated beam (RPLCB) is proposed, and the degree of coherence of RPLCB is described by Lorentz function. The matrix elements of RPLCB in anisotropic turbulent ocean are obtained. The intensity and polarization of RPLCB are studied via numerical simulations. The evolution of intensity of RPLCB in free space will evolve from ring shape into Lorentz shape caused by Lorentz function, and the Lorentz shape of RPLCB in turbulent ocean will be destroyed by turbulence and become a Gaussian profile at the longer distance. The RPLCB with a smaller coherence length will turn into Lorentz shape faster on propagation. The degree of polarization of RPLCB will decrease as distance increases, and the depolarization of RPLCB in turbulent ocean is more obvious than the same RPLCB in free space.

Authors

Institutions

Publication Details

Journal
Physica Scripta
Published
2025-03-05
DOI
https://doi.org/10.1088/1402-4896/adbce6
Primary Topic
Orbital Angular Momentum in Optics
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Research on characteristics of radially polarized Lorentz correlated beam in anisotropic turbulent ocean

Guiqiu Wang, Dajun Liu, Yaochuan Wang, Rui Cong et al.
Physica Scripta
Orbital Angular Momentum in Optics
article

Research on characteristics of radially polarized Lorentz correlated beam in anisotropic turbulent ocean

Guiqiu Wang, Dajun Liu, Yaochuan Wang, Rui Cong, Haiyang Zhong, Yan Yin
article en

Abstract

Abstract The cross-spectral density (CSD) matrix of radially polarized Lorentz correlated beam (RPLCB) is proposed, and the degree of coherence of RPLCB is described by Lorentz function. The matrix elements of RPLCB in anisotropic turbulent ocean are obtained. The intensity and polarization of RPLCB are studied via numerical simulations. The evolution of intensity of RPLCB in free space will evolve from ring shape into Lorentz shape caused by Lorentz function, and the Lorentz shape of RPLCB in turbulent ocean will be destroyed by turbulence and become a Gaussian profile at the longer distance. The RPLCB with a smaller coherence length will turn into Lorentz shape faster on propagation. The degree of polarization of RPLCB will decrease as distance increases, and the depolarization of RPLCB in turbulent ocean is more obvious than the same RPLCB in free space.

Physica ScriptaVol. 100(4)
Dalian Maritime University (CN)
National Natural Science Foundation of China
Life below water
Openalex Percentile: Top 97%
Orbital Angular Momentum in Optics
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.