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Development of an ultra-high precision X-ray telescope with an adaptive optics system

机译:开发具有自适应光学系统的超高精度X射线望远镜

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We are developing an ultra high precision Soft X-ray telescope. The design of the telescope is a normal incident one for 13.5nm band using Mo/Si multilayers. Two ideas are introduced. One is the optical measurement system in order to monitor the precision of the optics system. The other is the adaptive optics system with a deformable mirror, Using an X ray-optical separation filter, we can always monitor the deformation of the optics by optical light. With this information, we can control the deformable mirror to compensate the system deformation as a closed loop system. We confirmed that the absolute precision of the wave front sensor was less than 3 nm rms. The precision of the deformable mirror was roughly 5 nm rms. The shape of the primary mirror was an off-axis paraboloide with an effective diameter of 80mm. This primary mirror was coated by Mo/Si multilayers. The reflectivity of the primary mirror at 13.5nm was ranging from 30 to 50%. The X ray-optical separation filter was made from Zr with a thickness of ~170nm. The transmission of the filter for low energy X-ray was measured and was roughly 50 % at 13.5nm.
机译:我们正在开发超高精度的软X射线望远镜。望远镜的设计是使用Mo / Si多层的13.5nm波段的垂直入射。介绍了两个想法。一种是光学测量系统,以监视光学系统的精度。另一个是带有可变形反射镜的自适应光学系统,使用X射线光学分离滤镜,我们始终可以通过光学光来监视光学系统的变形。利用此信息,我们可以控制可变形反射镜以补偿系统闭环系统的变形。我们确认波前传感器的绝对精度小于3 nm rms。可变形反射镜的精度约为5 nm rms。主镜的形状是离轴抛物线,有效直径为80mm。该主镜被Mo / Si多层涂层。主镜在13.5nm处的反射率为30%至50%。 X射线光学分离滤光片由Zr制成,厚度约为170nm。测量了低能X射线滤光片的透射率,在13.5nm处约为50%。

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