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Aberrational interactions between axial and lateral misalignments in pupil-offset off-axis two-mirror astronomical telescopes

机译:瞳孔偏移轴向轴两镜子天文望远镜轴向和横向未对准之间的畸变相互作用

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摘要

Due to the absence of rotational symmetry, the effects of axial and lateral misalignments couple tightly together, which leads to special aberration field characteristics. This paper will present an in-depth and systematic discussion on the interactions between the effects of axial and lateral misalignments in pupil-offset off-axis two-mirror astronomical telescopes. The aberration function of this class of telescopes in the presence of axial and lateral misalignments is derived. The specific expressions of two dominant non-rotationally symmetric aberrations, i.e., astigmatism and coma, are obtained and the aberration field characteristics are discussed. Importantly, it is shown that under certain conditions, a node will arise in the field of view for these two kinds of aberrations. Then the aberrational compensation mechanisms between axial and lateral misalignments are quantitatively explicated, and it is shown that the non-rotationally symmetric aberrations induced by axial misalignments can well be compensated by lateral misalignments. However, we also find that in this process, the defocus aberration induced by these two kinds of misalignments will accumulate (rather than cancel out). Therefore, in practice, it is better to separate these two kinds of misalignment. Finally, we propose a simple method to decouple axial misalignments from lateral misalignments with wavefront measurement at one field position. Most of this work can be extended to other kind of pupil-offset off-axis astronomical telescopes, such as off-axis three-mirror anastigmatic telescopes. (C) 2019 Optical Society of America
机译:由于没有旋转对称性,轴向和横向未对准的影响紧密地耦合在一起,这导致特殊的像差场特征。本文将对瞳孔偏移偏离轴两镜子天文望远镜的轴向和横向未对准之间的相互作用进行深入和系统的讨论。这类伸缩件在轴向和横向未对准的情况下的像差函数是衍生的。获得两个主要非旋转对称像差,即散光和彗形差的特定表达,并且讨论了像差场特征。重要的是,显示在某些条件下,在这两种像差的视野中会出现节点。然后定量地阐述轴向和横向未对准之间的畸变补偿机制,并且示出了通过轴向错位引起的非旋转对称像差可以通过横向未对准来补偿。但是,我们还发现,在这个过程中,这两种错位引起的散焦像差将积聚(而不是取消)。因此,在实践中,最好分离这两种未对准。最后,我们提出了一种简单的方法,可以在一个场位置与波前测量的横向未对准与横向未对准进行轴向错位。大部分工作都可以扩展到其他类型的瞳孔偏移的轴外天文望远镜,如轴外三镜子腹围伸缩望远镜。 (c)2019年光学学会

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  • 来源
    《Applied optics》 |2019年第28期|共15页
  • 作者单位

    Chinese Acad Sci Changchun Inst Opt Fine Mech &

    Phys Changchun 130033 Jilin Peoples R China;

    Chinese Acad Sci Changchun Inst Opt Fine Mech &

    Phys Changchun 130033 Jilin Peoples R China;

    Chinese Acad Sci Changchun Inst Opt Fine Mech &

    Phys Changchun 130033 Jilin Peoples R China;

    Chinese Acad Sci Changchun Inst Opt Fine Mech &

    Phys Changchun 130033 Jilin Peoples R China;

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  • 正文语种 eng
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