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Manufacture of the combined primary and tertiary mirrors of the Large Synoptic Survey Telescope

机译:大型天气观测望远镜组合主,三面镜的制造

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The Steward Observatory Mirror Lab is nearing completion of the combined primary and tertiary mirrors of the Large Synoptic Survey Telescope. Fabrication of the combined mirror requires simulation of an active-optics correction that affects both mirror surfaces in a coordinated way. As is common for large mirrors, the specification allows correction of large-scale figure errors by a simulated bending of the substrate with the 156 mirror support actuators. Any bending affects both mirrors, so this active-optics correction is constrained by the requirement of bending the substrate so both mirrors meet their figure specifications simultaneously. The starting point of the simulated correction must be measurements of both mirrors with the substrate in the same shape, i. e. the same state of mechanical and thermal stress. Polishing was carried out using a 1.2 m stressed lap for smoothing and large-scale figuring, and a set of smaller passive rigid-conformal laps on an orbital polisher for deterministic small-scale figuring. The primary mirror is accurate to about 25 nm rms surface after the active-optics correction, while work continues toward completion of the tertiary.
机译:Steward天文台镜实验室即将完成大型天气观测望远镜的主,三面镜组合。组合镜的制造需要模拟主动光学校正,该校正会以协调的方式影响两个镜面。与大型反射镜一样,该规范允许通过使用156个反射镜支撑致动器对基板进行模拟弯曲来校正大规模图形误差。任何弯曲都会影响两个反射镜,因此这种主动光学校正受弯曲基板的要求所约束,因此两个反射镜同时满足其图形规格。模拟校正的起点必须是两个反射镜的测量值,并且基板的形状相同,即: e。机械应力和热应力处于相同状态。抛光使用1.2 m应力研磨圈进行平滑和大规模修形,并在轨道抛光机上使用一组较小的被动刚性保形研磨圈进行确定性的小型成型。主动光学校正后,主反射镜的表面精度约为25纳米rms,而第三镜的工作仍在继续。

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