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Test system for a Shack-Hartmann sensor based telescope alignment demonstrated at the 40cm Wendelstein Telescope

机译:40厘米的温德尔斯坦望远镜演示了基于Shack-Hartmann传感器的望远镜对准测试系统

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A commercial Shack-Hartman wavefront sensor is being used in a test setup installed at the Wendelstein 40 cmtelescope to test methods for telescope alignment based on reverse optimization. Measured low-order Zernikewave-fronts are being used to determine the misalignment of the telescopes optical elements. Then a procedureto optimize wave-front performance by aligning the telescope secondary mirror is applied.The setup contains a collimating optical system, the Shack-Hartman sensor and a guiding and acquisitioncamera.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:Wendelstein 40厘米望远镜安装的测试装置中使用了商用Shack-Hartman波前传感器,以测试基于反向优化的望远镜对准方法。测得的低阶Zernikewave锋面用于确定望远镜光学元件的未对准情况。然后应用通过对准望远镜副镜优化波前性能的程序,该装置包含一个准直光学系统,Shack-Hartman传感器以及一个引导和采集相机。(2012)COPYRIGHT光电仪器工程师协会(SPIE) )。摘要的下载仅允许个人使用。

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