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akaturk Akademik ölçüm

Makale detayı · 2009

M^2-factor of coherent and partially coherent dark hollow beams propagating in turbulent atmosphere

Dergi

Optics Express
OpenAlex Açık erişim · gold SJR Q1 JCR Q1 Atıf 143 Üst %10 Yüzdelik 99.0% FWCI 10.17
Yıl
2009
Tür
article

Veri kaynağı ayrımı

  • YÖKSİS dergi adı Optics Express
  • OpenAlex OpenAlex zenginleştirmesi (özet, atıf, konular)

Özet

OpenAlex · İngilizce

Analytical formula is derived for the M(2)-factor of coherent and partially coherent dark hollow beams (DHB) in turbulent atmosphere based on the extended Huygens-Fresnel integral and the second-order moments of the Wigner distribution function. Our numerical results show that the M(2)- factor of a DHB in turbulent atmosphere increases on propagation, which is much different from its invariant properties in free-space, and is mainly determined by the parameters of the beam and the atmosphere. The relative M(2)-factor of a DHB increases slower than that of Gaussian and flat-topped beams on propagation, which means a DHB is less affected by the atmospheric turbulence than Gaussian and flat-topped beams. Furthermore, the relative M(2)-factor of a DHB with lower coherence, longer wavelength and larger dark size is less affected by the atmospheric turbulence. Our results will be useful in long-distance free-space optical communications.

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143 atıf

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