Off-axis aberration correction for a wide field scanning telescope

Charles P. Scott, B. Potsaid, J. Wen
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引用次数: 1

Abstract

Due to the tradeoff between field of view and resolution, the ability of traditional optical telescopes to obtain high-resolution wide field images is limited. This work presents a design for a scanning optical telescope that can produce high resolution images over a wide field of view. This is accomplished by scanning one of the telescope's optical elements. Inherent in such a design is the introduction of optical aberrations as off-axis scanning occurs. The deformable mirror technology is implemented to adaptively correct these aberrations such that on-axis resolution is achieved at off-axis scan angles. The optical design layout is optimized in software to minimize on-axis wavefront aberrations. This paper presents results involving two deformable mirrors based on different technologies: the AgilOptics mirror based on electrostatic actuators and the Imagine Optic mirror based on electromagnetic actuators. Both mirrors are similar in size (about 15mm aperture), but the Imagine Optic mirror has significantly larger actuator displacement, though at a higher cost. The static telescope design has a field of view of 0.49-degrees which is increased to 20-degrees with the AgilOptics mirror and 40-degrees with the Imagine Optic mirror.
宽视场扫描望远镜的离轴像差校正
由于视场和分辨率之间的权衡,传统光学望远镜获得高分辨率宽视场图像的能力受到限制。这项工作提出了一种扫描光学望远镜的设计,它可以在宽视场上产生高分辨率的图像。这是通过扫描望远镜的一个光学元件来完成的。这种设计中固有的是在离轴扫描发生时引入光学像差。采用可变形反射镜技术自适应校正这些像差,从而在离轴扫描角度下实现轴上分辨率。在软件中优化了光学设计布局,以最小化轴上波前像差。本文介绍了两种基于不同技术的变形镜的结果:基于静电致动器的AgilOptics反射镜和基于电磁致动器的Imagine Optic反射镜。两种反射镜的尺寸相似(孔径约为15毫米),但Imagine Optic反射镜的执行器位移明显更大,尽管成本更高。静态望远镜设计的视场为0.49度,使用AgilOptics反射镜增加到20度,使用Imagine Optic反射镜增加到40度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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