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High-contrast imager for Complex Aperture Telescopes (HiCAT). 4. Status and wavefront control development

机译:复杂孔径望远镜(HICAT)的高对比度成像仪。 4.状态和波前控制开发

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Segmented telescopes are a possible approach to enable large-aperture space telescopes for the direct imaging and spectroscopy of habitable worlds. However, the increased complexity of their aperture geometry, due to their central obstruction, support structures and segment gaps, makes high-contrast imaging very challenging. The High-contrast imager for Complex Aperture Telescopes (HiCAT) was designed to study and develop solutions for such telescope pupils using wavefront control and starlight suppression. The testbed design has the flexibility to enable studies with increasing complexity for telescope aperture geometries starting with off-axis telescopes, then on-axis telescopes with central obstruction and support structures (e.g. the Wide Field Infrared Survey Telescope [WFIRST]), up to on-axis segmented telescopes e.g. including various concepts for a Large UV, Optical, IR telescope (LUVOIR), such as the High Definition Space Telescope (HDST). We completed optical alignment in the summer of 2014 and a first deformable mirror was successfully integrated in the testbed, with a total wavefront error of 13nm RMS over a 18mm diameter circular pupil in open loop. HiCAT will also be provided with a segmented mirror conjugated with a shaped pupil representing the HDST configuration, to directly study wavefront control in the presence of segment gaps, central obstruction and spider. We recently applied a focal plane wavefront control method combined with a classical Lyot coronagraph on HiCAT, and we found limitations on contrast performance due to vibration effect. In this communication, we analyze this instability and study its impact on the performance of wavefront control algorithms. We present our Speckle Nulling code to control and correct for wavefront errors both in simulation mode and on testbed mode. This routine is first tested in simulation mode without instability to validate our code. We then add simulated vibrations to study the degradation of contrast performance in the presence of these effects.
机译:分段望远镜一种可能的方法来启用直接成像大孔径空间望远镜和可居住世界的光谱学。然而,它们的孔径的几何形状的增加的复杂性,由于它们的中心阻塞,支撑结构和片段间隙,使得高对比度成像非常具有挑战性。复杂孔径望远镜(HiCAT)的高对比度成像的目的是研究和开发使用波前控制和星光抑制这种望远镜的学生解决方案。该试验台的设计具有灵活性,使研究,用于启动具有离轴望远镜望远镜孔径的几何形状增加的复杂性,则在轴望远镜具有中央阻碍物和支撑结构(例如,宽视场红外观测望远镜[WFIRST]),至多上轴分段望远镜如包括用于大型UV,光,IR望远镜(LUVOIR)各种概念,如高清晰度太空望远镜(HDST)。我们完成了光学对准在2014年夏季和第一可变形镜被成功地集成在测试平台,有超过在开环一个直径18mm的圆形光瞳为13nm RMS的总波前误差。 HiCAT也将设置有与代表HDST结构的形状的光瞳共轭的分割镜,直接研究在片段间隙,中央阻碍物和蜘蛛的存在下波阵面控制。我们最近采用焦平面波面控制方法与HiCAT经典李奥日冕相结合,我们发现在对比度表现,由于振动效果的局限性。在这个沟通,我们分析这种不稳定性,并研究其对波前控制算法的性能影响。我们提出我们的斑点归零码来控制和纠正无论是在模拟模式和实验平台模式的波前误差。该程序在仿真模式首先测试不稳定性,以验证我们的代码。然后,我们添加模拟振动来研究这些效应的存在对比度性能的下降。

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