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Decreasing the Inner Working Angle in High-Contrast Imaging by Pupil Replication

机译:通过瞳孔复制降低高对比度成像的内部工作角度

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Imaging for exo-planet detection requires both high contrast and a small inner working angle. We show that, for several of the techniques proposed so far to achieve this, the inner working angle can be reduced by adding pupil replication between the telescope and the high contrast imaging system. Using pupil replication, the on-axis image of the star is decreased to a size smaller than the diffraction limit of the telescope, and off axis the point spread function of the planet undergoes minor changes, contained within the envelope of the point spread function of the telescope; the spectrum remains unchanged. The principle of pupil replication was proven experimentally and can be effected by a small-sized, high throughput optical system added between the telescope and the high contrast imaging system. High contrast imaging systems to which pupil replication has been found to be applicable so far include apodisation techniques like pupil apodisation, aperture masks, image plane masks, coronagraphs and combinations. Mathematical assessment and simulations of the sensitivity of pupil replication to optical errors show that the requirements for this system are the same as those for the primary telescope - pupil replication effectively remaps the output pupil of the telescope to the input pupil of the high contrast imaging system. Our results in this paper aim to show, in a realistic set-up, the feasibility of an improvement of the inner working angle by a factor of 4 using four-fold replication optics while maintaining the contrast performance. We do this through analysis of the pupil replication principle including off axis behavior when applied to high contrast imaging systems using pupil apodisation or a shaped mask. We specifically look at the situations similar to that of the Terrestrial Planet Finder Coronagraph and Darwin. We found that an inner working angle of 30 mas can be achieved with a contrast of 10~(-10) and a large field of view without increasing the requirements except for the pointing.
机译:用于系外行星检测的成像既需要高对比度又需要较小的内部工作角度。我们表明,到目前为止,为实现此目的而提出的几种技术,可以通过在望远镜和高对比度成像系统之间增加瞳孔复制来减小内部工作角度。使用光瞳复制,恒星的轴上图像减小到小于望远镜的衍射极限的大小,离轴,行星的点扩散函数发生微小变化,包含在点扩散函数的包络内望远镜频谱保持不变。光瞳复制的原理已通过实验证明,并且可以通过在望远镜和高对比度成像系统之间添加的小型高通量光学系统来实现。迄今为止发现瞳孔复制可应用的高对比度成像系统包括变迹技术,例如瞳孔变迹,光圈掩模,像面掩模,冠冕仪及其组合。数学评估和模拟瞳孔复制对光学误差的敏感性表明,该系统的要求与主望远镜的要求相同-瞳孔复制有效地将望远镜的输出瞳孔重新映射到高对比度成像系统的输入瞳孔。我们在本文中的结果旨在显示出一个现实的设置,即使用四倍复制光学器件将内部工作角度提高4倍,同时保持对比度性能的可行性。我们通过对瞳孔复制原理的分析来做到这一点,包括应用于使用瞳孔变迹或成形掩模的高对比度成像系统时的偏轴行为。我们专门研究与地球行星搜索仪日冕仪和达尔文类似的情况。我们发现,在没有增加要求的情况下,除了指向之外,在10〜(-10)的对比度和较大的视野范围内可以实现30 mas的内部工作角度。

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