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EUV Imaging Experiment of an Adaptive Optics Telescope

机译:自适应光学望远镜的EUV成像实验

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We report an experimental result of our normal-incident EUV telescope tuned to a 13.5 nm band, with an adaptive optics. The optics consists of a spherical primary mirror and a secondary mirror. Both are coated by Mo/Si multilayer. The diameter of the primary and the secondary mirrors are 80 mm and 55mm, respectively. The secondary mirror is a deformable mirror with 31 bimorph-piezo electrodes. The EUV from a laser plasma source was exposed to a Ni mesh with 31 micro-m wires. The image of this mesh was obtained by a back-illuminated CCD. The reference wave was made by an optical laser source with 1 μm pin-hole. We measure the wave form of this reference wave and control the secondary mirror to get a good EUV image. Since the paths of EUV and the optical light for the reference were different from each other, we modify the target wave from to control the deformable mirror, as the EUV image is best. The higher order Zernike components of the target wave form, as well as the tilts and focus components, were added to the reference wave form made by simply calculated. We confirmed the validity of this control and performed a 2.1 arc-sec resolution.
机译:我们报告了使用自适应光学器件将我们的正常入射EUV望远镜调谐到13.5 nm波段的实验结果。光学器件由球面主镜和副镜组成。两者均涂覆有Mo / Si多层膜。主镜和副镜的直径分别为80毫米和55毫米。副镜是具有31个双压电晶片电极的可变形镜。将来自激光等离子体源的EUV暴露于具有31微米线的Ni网中。该网格的图像是通过背照式CCD获得的。参考波是由具有1μm针孔的光学激光源发出的。我们测量该参考波的波形并控制辅助反射镜以获得良好的EUV图像。由于EUV的路径和作为参考的光互不相同,因此我们将目标波从修改为控制可变形反射镜,因为EUV图像效果最佳。将目标波形的高阶Zernike分量以及倾斜和聚焦分量添加到通过简单计算得出的参考波形中。我们确认了此控件的有效性,并执行了2.1弧秒的分辨率。

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