首页> 外文会议>Conference on Optical Measurement Systems for Industrial Inspection >Remote sensing catadioptric telescope corrector lens design for facilitating measurement of center thickness and air gaps of inner lenses using low-coherence interferometry
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Remote sensing catadioptric telescope corrector lens design for facilitating measurement of center thickness and air gaps of inner lenses using low-coherence interferometry

机译:遥感透镜矫正器透镜设计,用于使用低相干干涉测量促进内透镜中心厚度和空气差距的测量

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Whether the center thickness and air gaps of the inner lens can be measured during lens assembly depends on the configuration of the entire lens assembly. The corrector lens of a conventional remote sensing catadioptric telescope generates divergent optical information because of its negative diopter lens constructions. Consequently, the center thickness of the lenses and center air gaps between lens interfaces cannot be easily measured. This can be solved by equipping a positive diopter lens on the image side during remote sensing catadioptric telescope lens optimization and by measuring the center thickness and air gap of the lens from the image side through low-coherence interferometry. The results of this study indicate that the optical signals and air gap interfaces of four lens elements can be clearly identified using low-coherence interferometry and that the center thickness and air gap interfaces of lenses can be calculated accurately.
机译:在透镜组件期间可以测量内透镜的中心厚度和空气间隙是否取决于整个透镜组件的配置。 传统遥感射频望远镜的校正透镜由于其负屈光度镜片结构而产生发散光学信息。 因此,透镜界面之间的透镜和中心空气间隙的中心厚度不能轻易测量。 这可以通过在遥感射频望远镜镜头优化期间装配在图像侧的正屈光度镜头来解决,并且通过低相干干涉法测量从图像侧的透镜的中心厚度和空气间隙。 该研究的结果表明,可以使用低相干干涉测量法清楚地识别四个透镜元件的光信号和空气间隙界面,并且可以精确地计算透镜的中心厚度和空气间隙界面。

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