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利用图像畸变进行正射校正的光学设计。

Optical design using image distortion for orthorectification.

作者信息

Johnson Tim P, Sasian Jose, Cook Lacy G

出版信息

Appl Opt. 2020 Aug 1;59(22):G175-G184. doi: 10.1364/AO.392302.

Abstract

Imaging the curved Earth from above typically results in a distorted image with reduced spatial resolution near the edge of the field. The effect is proportional to the field of view (FOV) and altitude. It is similar to the negative (barrel) distortion common in fish-eye lenses, but is due here to the convex object and not the optical system. Although image processing methods exist to partially correct for negative distortion, the reduced spatial resolution near the edge of the field is unrecoverable. Instead this can be corrected for optically by inducing the right amount of positive distortion into the optical design. The amount of positive distortion required to counter the negative distortion from the curved Earth is calculated as a function of FOV and altitude. An optical system with positive distortion is more challenging to design than with negative distortion as this increases the FOV in image space and requires a larger focal plane array. An off-axis, all-reflective design with /2.5, 2.5 in. effective focal length, 70×4 FOV, +13 distortion is shown that could be used as a push-broom satellite sensor in a polar orbit with constant spatial resolution.

摘要

从上方对弯曲的地球进行成像通常会导致图像失真,视野边缘附近的空间分辨率降低。这种效应与视场(FOV)和高度成正比。它类似于鱼眼镜头中常见的负(桶形)畸变,但在此处是由凸形物体而非光学系统导致的。尽管存在图像处理方法来部分校正负畸变,但视野边缘附近降低的空间分辨率是无法恢复的。相反,可以通过在光学设计中引入适量的正畸变来进行光学校正。抵消来自弯曲地球的负畸变所需的正畸变量是根据视场和高度来计算的。设计具有正畸变的光学系统比具有负畸变的光学系统更具挑战性,因为这会增加图像空间中的视场并需要更大的焦平面阵列。展示了一种离轴全反射设计,其有效焦距为2.5英寸,视场为70×4,畸变为+13,可作为极轨上具有恒定空间分辨率的推扫式卫星传感器。

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