拼接式望远镜主镜衍射效应研究

Research on diffraction effect of primary mirror in segmented telescope

  • 摘要: 拼接式主镜的设计使超大口径望远镜的构想成为现实。为了研究拼接式望远镜的成像性能,精确分析和量化了拼接式主镜构型、平移误差、倾斜误差对衍射效应的影响,从拼接式光学系统的成像原理出发,基于齐次坐标变换建立了拼接式主镜的光瞳模型,并仿真分析了拼接主镜构型对衍射效应的影响。分析结果表明:对于不同构型的拼接主镜,其衍射效应受拼接主镜的填充因子和孔径间隔共同影响,填充因子越高,孔径间隔越小,系统成像质量越好。以典型的拼接主镜构型为例,分别仿真分析了单个子镜平移误差、倾斜误差和拼接主镜整体平移误差、倾斜误差对衍射效应的影响。分析结果表明:对于单个子镜,平移误差对远场衍射的影响具有周期性;对于拼接主镜整体,当子镜piston误差的均方根值小于0.039λ时,斯特列尔比大于0.95;当子镜tip-tilt误差的均方根值小于0.036λ时,斯特列尔比大于0.95。分析结果为拼接式望远镜的成像性能分析、主镜的构型设计、平移误差和倾斜误差的检测与调整等提供了依据。

     

    Abstract: The design of the segmented primary mirror makes an idea of the extremely large aperture telescope a reality. In order to study the imaging performance of the segmented telescope, the effect of the segmented primary mirror configuration, translation error, and tilt error on diffraction effect was precisely analyzed and quantified. Based on the imaging principle of the segmented optical system, the pupil models of the segmented primary mirror were established based on the homogeneous coordinate transformation. And the effect of the segmented primary mirror configuration on the diffraction effect was simulated and analyzed. The analysis results show that for the segmented primary mirrors with different configurations, the diffraction effect is affected by the fill factor and the aperture interval of the segmented primary mirror, the higher the fill factor, the smaller the aperture interval, and the better the system imaging quality. Taking the typical segmented primary mirror configuration as an example, the effect of the translation error and tilt error of the single sub-mirror and the overall translation error and tilt error of the segmented primary mirror on diffraction effect was simulated and analyzed, respectively. The analysis results show that for the single sub-mirror, the effect of the translation error on far-field diffraction is periodic. And for the overall segmented primary mirror, the Strehl ratio is higher than 0.95, when the root mean square of the sub-mirror piston error is less than 0.039λ, or the root mean square of the sub-mirror tip-tilt error is less than 0.036λ. The analysis results provide the basis for the imaging performance analysis of the segmented telescope, the configuration design of the primary mirror, and the detection and adjustment of the translation error and tilt error.

     

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