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An Image Telecentric Optical System of Low-distortion and Wide-field

机译:低失真和宽场的图像远心光学系统

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In the final step of approaching and docking proximity of space rendezvous and docking, it is necessary to measure therelative position and posture of two spacecrafts with high precision using by optical imaging sensor. The image quality ofthe optical system itself of optical image sensor, to a great extent, will influence the accuracy of navigation information ofrendezvous and docking, and even determine the success or failure of rendezvous and docking task. The image telecentricoptical system, adopted by the multi-components and retrofocus structure and designed by the hyperfocal distance theory,not only can realize clear imaging from 2 meters to infinity, but also can make sure the center position of image that isimaged by the object from 2 meters to infinity basically invariant. It used the method of "S" type correction of distortionand corrected the distortion of edged field of view (FOV) and 0.8 FOV synchronously, which realized the relative distortionless than 0.028%(absolute distortion less than 0.78 )in the range of μm 30° fields of view, and met the requirements ofthe high precision of imaging system and illuminancy uniformity of different fields of view.
机译:在接近和对接的空间聚会和对接附近的最后步骤中,有必要测量通过光学成像传感器具有高精度的两个航天器的相对位置和姿势。图像质量光学系统本身的光学图像传感器在很大程度上会影响导航信息的准确性结识和对接,甚至确定了会合和对接任务的成功或失败。图像远心光学系统,由多分量和回析焦结构采用,由超学院距离理论设计,不仅可以实现2米到无限的清晰成像,还可以确保图像的中心位置由2米到Infinity的对象成像基本不变。它使用了“S”类型校正的失真方法并同步地纠正了边缘视野(FOV)和0.8 FOV的变形,从而实现了相对失真小于0.028%(绝对失真小于0.78),范围为μm30°的视野,并满足要求的要求不同视野的成像系统的高精度和照明均匀性。

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