Propagation factor of electromagnetic concentric rings Schell-model beams in non-Kolmogorov turbulence

doi:10.1088/1674-1056/26/2/024201

Abstract

We derive an analytical expression for the propagation factor (known as M²-factor) of electromagnetic concentric rings Schell-model (EM CRSM) beams in non-Kolmogorov turbulence by utilizing the extended Huygens-Fresnel diffraction integral formula and the second-order moments of the Wigner distribution function (WDF). Our results show that the EM CRSM beam has advantage over the scalar CRSM beam for reducing the turbulence-induced degradation under suitable conditions. The EM CRSM beam with multi-rings far-fields in free space is less affected by the turbulence than the one with dark-hollow far-fields or the electromagnetic Gaussian Schell-model (EGSM) beam. The dependence of the M²-factor on the beam parameters and the turbulence are investigated in detail.

Keywords: atmospheric propagation partial coherence atmospheric turbulence

Received: 19 September 2016
Revised: 27 October 2016
Accepted manuscript online:

PACS:	42.25.Dd	(Wave propagation in random media)
	42.25.Kb	(Coherence)
	42.68.Bz	(Atmospheric turbulence effects)

Fund:

Project supported by the National Basic Research Program of China (Grant No. 2013CBA01702), the National Natural Science Foundation of China (Grant Nos. 61377016, 11104049, 10974039, 61575055, and 61575053), the Fundamental Research Funds for the Central Universities, China (Grant No. HIT.BRETIII.201406), and the Program for New Century Excellent Talents in University, China (Grant No. NCET-12-0148).

Corresponding Authors: Shu-Tian Liu
E-mail: stliu@hit.edu.cn

Cite this article:

Zhen-Zhen Song(宋真真), Zheng-Jun Liu(刘正君), Ke-Ya Zhou(周可雅), Qiong-Ge Sun(孙琼阁), Shu-Tian Liu(刘树田) Propagation factor of electromagnetic concentric rings Schell-model beams in non-Kolmogorov turbulence 2017 Chin. Phys. B 26 024201

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Propagation factor of electromagnetic concentric rings Schell-model beams in non-Kolmogorov turbulence

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