首页> 外文会议>Conference on UV, Optical, and IR Space Telescopes and Instruments 29-31 March 2000 Munich, Germany >Initial test results from the Next Generation Space Telescope (NGST) wavefront sensing and control testbed (WCT)
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Initial test results from the Next Generation Space Telescope (NGST) wavefront sensing and control testbed (WCT)

机译:下一代太空望远镜(NGST)波前传感和控制测试台(WCT)的初步测试结果

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This paper describes the results of a few of the initial series of tests being conducted with the first configuration of the Next Genration Space Telescope (NGST) Wavefront sensing and Control Testbed (WCT1). WCT1 is a 1:1, f/16.6 re-imaging system, incorporating two deformable mirrors (DM) located at pupil conjugate positions with 6 actuators/diameter (SM/DM) and 20 actuators/diameter (AO/DM). A CCD on a precision stage is used for obtaining deforcused images providing phase diversity for wavefront determination using phase retrieval. In a typical experiment, wavefront error (WFE) is injected into the optical path with the SM/DM and then corrected using he more densely actuated AO/DM. Wavefront analysis is provided via a phase retrieval agorithm, and control software is used to reshape the AO/DM and corect the wavefront. A summary of the results of some initial tests are presented.
机译:本文介绍了使用下一代空间望远镜(NGST)波前传感和控制测试台(WCT1)的第一配置进行的一系列初始测试的结果。 WCT1是1:1,f / 16.6的重新成像系统,在两个瞳孔共轭位置(SM / DM)和20个促动器/直径(AO / DM)中,在瞳孔共轭位置装有两个可变形反射镜(DM)。精密平台上的CCD用于获得变形图像,从而提供相位分集,以便使用相位检索来确定波前。在典型的实验中,将波前误差(WFE)与SM / DM一起注入光路,然后使用密度更高的AO / DM进行校正。波前分析通过相位检索算法提供,控制软件用于重塑AO / DM并固定波前。总结了一些初始测试的结果。

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