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Spectral shifts of partially coherent radial array beams passing through ABCD optical systems

机译:穿过ABCD光学系统的部分相干径向阵列光束的光谱偏移

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摘要

The expressions for the spectral intensity of partially coherent Gaussian Schell-model (GSM) radial array beams for both the correlated and uncorrelated superpositions passing through ABCD optical systems have been derived by using the extended Huygens-Fresnel diffraction integral. The effects of the normalized radius R, the number of beamlets N, the spatial coherent parameter of array beamlets beta and the optical system parameters on the on-axis and off-axis relative spectral shifts for the two types of superposition have been discussed in detail. The results show that for the correlated superposition, the on-axis spectral intensity in free space and the off-axis spectral intensity on the geometrical focal plane depends on the source spectral density S~(0)(omega), the spatial coherent parameter of array beamlets beta, the generalized Fresnel number of the system F, the normalized radius R and the number of beamlets N, whereas the spectral intensity for the uncorrelated superposition is independent of the number of beam-lets N. Furthermore, as for on the actual focal plane, the off-axis spectral intensity for the two types of superposition is closely related to N.
机译:通过使用扩展的惠更斯-菲涅耳衍射积分,导出了部分相干高斯谢尔模型(GSM)径向阵列光束通过ABCD光学系统时相关和不相关叠加的光谱强度表达式。讨论了归一化半径R,子束数N,阵列子束β的空间相干参数以及光学系统参数对两种叠加类型的轴上和轴外相对光谱偏移的影响。 。结果表明,对于相关叠加,自由空间的轴上光谱强度和几何焦平面上的轴外光谱强度取决于源光谱密度S〜(0)(ω),空间相干参数。阵列子束beta,系统的广义菲涅尔数F,归一化半径R和子束N的数量,而不相关叠加的光谱强度与子束N的数量无关。此外,关于实际在焦平面上,两种叠加类型的离轴光谱强度与N密切相关。

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