Temporal-frequency spectra for optical wave propagating through non-Kolmogorov turbulence

被引:40
作者
Du, Wenhe [1 ,2 ]
Tan, Liying [1 ]
Ma, Jing [1 ]
Jiang, Yijun [1 ]
机构
[1] Harbin Inst Technol, Natl Key Lab Tunable Laser Technol, Harbin 150001, Peoples R China
[2] Qiqihar Univ, Coll Sci, Qiqihar 161006, Peoples R China
基金
中国国家自然科学基金;
关键词
STAR IMAGE MOTION; ANGLE-OF-ARRIVAL; ATMOSPHERIC-TURBULENCE; STRATOSPHERIC TURBULENCE; FLUCTUATIONS; SCALE; FLUID;
D O I
10.1364/OE.18.005763
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Nowadays it has been accepted that the Kolmogorov model is not the only possible turbulent one in the atmosphere, which has been confirmed by the increasing experimental evidences and some results of theoretical investigation. This has prompted the scientist community to study optical propagation in non-Kolmogorov atmospheric turbulence. In this paper, using a non-Kolmogorov power spectrum which has a more general power law instead of standard Kolmogorov power law value 11/3 and a more general amplitude factor instead of constant value 0.033, the temporal power spectra of the presentative amplitude and phase effects, irradiance and angle of arrival fluctuations, have been derived for horizontal link in weak turbulence. And then the influence of spectral power-law variations on the temporal power spectrum has been analyzed. It is anticipated that this work is helpful to the investigations of atmospheric turbulence and optical wave propagation in the atmospheric turbulence. (C) 2010 Optical Society of America
引用
收藏
页码:5763 / 5775
页数:13
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