共查询到14条相似文献,搜索用时 156 毫秒
1.
推导出部分相干厄米-双曲正弦-高斯(H-ShG)光束通过湍流大气的平均光强和角扩展的解析表示式,并用以研究了部分相干H-ShG光束在湍流中的平均光强分布演化和角扩展. 结果表明,折射率结构常数C2n的增加和空间相关长度σ0的减小都会加速演化过程. 引入相对角扩展来定量描述光束抗拒湍流的能力. 空间相关长度σ0,束腰宽度w0和双曲
关键词:
平均光强分布演化
角扩展
湍流大气
部分相干厄米-双曲正弦-高斯(H-ShG)光束 相似文献
2.
基于广义惠更斯-菲涅尔原理,并采用将部分相干双曲余弦高斯光束用厄米-高斯光束的非相干叠加表示的方法,研究了部分相干双曲余弦高斯光束通过湍流大气的光束扩展问题,推导出了部分相干双曲余弦高斯光束通过湍流大气均方根束宽的解析表达式.研究表明,部分相干双曲余弦高斯光束的扩展随着湍流大气的折射率结构常数C2n和光束离心参数δ的增大而加剧.但是,随着δ的增大,部分相干双曲余弦高斯光束受到湍流的影响减小.
关键词:
部分相干双曲余弦高斯光束
湍流大气
光束扩展 相似文献
3.
推导出了部分相干双曲余弦高斯光束在自由空间和湍流大气中传输瑞利区间的解析公式,并研究了湍流对光束瑞利区间的影响.研究表明,部分相干双曲余弦高斯光束的瑞利区间由湍流强度和光束参数等因数共同确定.湍流使得光束的瑞利区间缩短,并且湍流越强瑞利区间越短.在自由空间中,瑞利区间随光束相干参数 α 、光束参数 β 和高斯束宽 w 0的增大以及波长 λ 的减小而增大.但是, α,β 和 w 0越小以及 λ 越大,瑞利区间受湍流的影响越小.并且,当
关键词:
瑞利区间
部分相干双曲余弦高斯光束
大气湍流
自由空间 相似文献
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采用积分变换的技巧,推导出了径向分布高斯列阵光束通过湍流大气传输的二阶矩束宽和远场发散角的解析公式,并详细研究了大气湍流对光束扩展和方向性的影响.研究表明,相干合成情况下,子光束数N越小、径向分布半径r0越大,列阵光束扩展受湍流影响越小.相干较非相干合成时列阵光束的扩展小,但非相干合成时列阵光束扩展受湍流的影响比相干合成时的小.特别地,N足够小或r0足够大时,相干与非相干合成列阵光束的远场束宽相等.另一方面,还给出了相干和非相干合成径向分布高斯列阵
关键词:
径向分布高斯列阵光束
大气湍流
相干和非相干合成
二阶矩束宽 相似文献
6.
厄米-高斯光束在非Kolmogorov大气湍流中的传输性质 总被引:1,自引:1,他引:0
基于广义惠更斯-菲涅尔原理和非Kolmogorov(非K)谱,推导出了厄米-高斯光束在非K大气湍流中传输的束宽、角扩展以及M2因子的解析表达式.数值计算表明,在传输距离比较远(如z≥3km)时,厄米-高斯光束的束宽、角扩展和M2因子随广义指数参量α的增大而增加直到α=3.11时达到最大值后再随α的增大而减小;随湍流的内尺度l0的减小而增大;随外尺度L0的增加而增大(3.6α4).但是当广义指数参量α在3α3.6区间取值时,束宽和M2因子几乎不随外尺度的增加而变化. 相似文献
7.
采用积分变换,推导出了双曲余弦高斯(ChG)列阵光束通过湍流大气传输的二阶矩束宽和角扩展的解析公式,给出了ChG列阵光束与一束高斯光束具有相同角扩展的条件。研究表明:相干合成的ChG列阵光束的角扩展比非相干合成的小,但是,非相干合成的ChG列阵光束的角扩展受湍流影响比相干合成ChG光束小;相干合成情况下,ChG列阵光束的角扩展随离心参数、束腰宽度和相对子光束间距的变化均出现振荡,但在湍流中的振荡减弱,非相干合成情况下,ChG列阵光束的角扩展与相对子光束间距和光束数无关。 相似文献
8.
采用积分变换,推导出了双曲余弦高斯(ChG)列阵光束通过湍流大气传输的二阶矩束宽和角扩展的解析公式,给出了ChG列阵光束与一束高斯光束具有相同角扩展的条件。研究表明:相干合成的ChG列阵光束的角扩展比非相干合成的小,但是,非相干合成的ChG列阵光束的角扩展受湍流影响比相干合成ChG光束小;相干合成情况下,ChG列阵光束的角扩展随离心参数、束腰宽度和相对子光束间距的变化均出现振荡,但在湍流中的振荡减弱,非相干合成情况下,ChG列阵光束的角扩展与相对子光束间距和光束数无关。 相似文献
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The closed-form expression for the angular spread of Gaussian Schell-model (GSM) array beams propagating through atmospheric
turbulence is derived. It is shown that the angular spread θ
sp of GSM array beams for the superposition of the cross-spectral density function is smaller than of those for the superposition
of the intensity. However, the θ
sp of GSM array beams for the superposition of the intensity is less sensitive to turbulence than that for the superposition
of the cross-spectral density function. For the superposition of the cross-spectral density function, θ
sp of GSM array beams with smaller coherence length σ
0, smaller waist width w
0, smaller beam number N, and larger separation distance x
d
are less affected by turbulence than of those with larger σ
0,w
0,N, and smaller x
d
; while, for the superposition of the intensity, the effect of turbulence on θ
sp is independent of N and x
d
. In addition, the angular spread is nearly the same for the two types of superposition when σ
0 or w
0 is small enough, or x
d
is large enough. On the other hand, it is found that there exist equivalent GSM array beams for the two types of superposition
which may have the same directionality as the corresponding fully coherent Gaussian beam in free space and also in turbulence. 相似文献
12.
Propagation of partially coherent beams carrying an edge dislocation through atmospheric turbulence along a slant path
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This paper derives the explicit expressions for the average intensity, beam width and angular spread of Gaussian Schell-model (GSM) beams with edge dislocation propagating through atmospheric turbulence along a slant path. The propagation of GSM beams with edge dislocation through horizontal atmospheric turbulence can be treated as a special case through a slant one. The propagation properties of GSM beams with edge dislocation through slant atmospheric turbulence are studied, where the influence of edge dislocation parameters including the slope p and off-axis distance d on the spreading of GSM beams with edge dislocation in atmospheric turbulence is stressed. It shows that the spreading of the intensity profile of GSM beams with edge dislocation along a slant path is smaller than that along a horizontal path in the long-distance atmospheric propagation. The larger the slope vert pvert and the smaller the off-axis distance vert dvert are, the less the beam-width spreading and angular spread of GSM beams with edge dislocation are affected by turbulence. The GSM beams with edge dislocation is less affected by turbulence than that of GSM beams without edge dislocation. The results are illustrated numerically and their validity is interpreted physically. 相似文献
13.
The spreading of partially coherent polychromatic Hermite-Gaussian (PCPHG) beams propagating through non-Kolmogorov turbulence is studied, where the effect of non-Kolmogorov turbulence and beam bandwidth on the beam width spreading and angular spread is stressed. It is shown that the variation of the relative beam width of PCPHG beams with the generalized exponent parameter of non-Kolmogorov turbulence is non-monotonic. The larger bandwidth of PCPHG beams is, the smaller the relative beam width and the smaller the relative angular spread. Therefore, PCPHG beams with larger bandwidth are less affected by non-Kolmogorov turbulence than those with smaller bandwidth. PCPHG beams are less sensitive to the effect of non-Kolmogorov turbulence than fully coherent polychromatic Hermite-Gaussian (FCPHG) beams and polychromatic Gaussian Schell-model (PGSM) beams. The results are illustrated by numerical examples and interpreted. 相似文献
14.
The closed-form expression for the mean-squared width of apertured partially coherent beams propagating through turbulent media is derived by using the integral transform technique. The influence of turbulence on the spreading of apertured partially coherent beams is studied quantitatively by examining the relative mean-squared width, which is defined as the ratio of the mean-squared width of an apertured partially coherent beam in turbulence to the mean-squared width of the same beam in free space. On the other hand, the range of turbulence-independent propagation, also a reasonable measure of the resistance of a beam to turbulence, is obtained by examining the mean-squared width. It is shown that the spreading of apertured partially coherent beams is less affected by turbulence with smaller truncation parameter δ and coherence parameter α than with larger δ and α. In addition, the influence of turbulence on the spreading of apertured partially coherent beams increases first and then decreases due to increasing waist width w0. The results obtained are explained physically. 相似文献