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Optimized mirror supports active primary mirrors and adaptive secondaries for the Optical Very Large Array (OVLA)

机译:优化的反射镜支持光学超大型阵列(OVLA)的活动主反射镜和自适应辅助反射镜

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Abstract: This article first deals with general aspects ofoptimizing mirror supports. A wide variety of supporttopologies have been optimized by Nelson et al forunobscured entrance pupils. Optical forces andlocations of point supports have been calculated herefor annular pupils. Efficient topologies introducing asmall amount of defocusing are also proposed forunobscured and annular pupils. Support efficiencies aregiven for each topology. Wavefront errors are estimatedin the case of a defective cell, in order to specifytolerances on forces and geometries. The OVLA activeoptics is then discussed. The very thin,meniscus-shaped primary will be actively supported by29 actuators and 3 fixed points. Actuator locations andforces have been calculated to minimize the mirrordeflection under its own weight but also to allow agood control of astigmatism. We finally present a studyof a concave adaptive secondary for the OVLAtelescopes. As an initial result, we propose a defocusadaptive corrector with a variable thicknessdistribution. Conditions of use are defined, andperformances are evaluated.!13
机译:摘要:本文首先讨论优化镜像支持的一般方面。尼尔森(Nelson)等人对入瞳进行了模糊处理,从而优化了各种支持拓扑。对于环形瞳孔,已经计算了点支撑件的光学力和位置。还提出了有效的拓扑结构,该结构引入了少量的散焦,用于未遮挡的环形瞳孔。每种拓扑都提供了支持效率。为了确定作用力和几何形状的公差,在单元损坏的情况下估计波前误差。然后讨论OVLA主动光学。 29个执行器和3个固定点将主动支撑非常薄的弯月形主线圈。计算了执行器的位置和作用力,以最大程度地减小其自身重量下的镜面偏转,但也可以很好地控制像散。最后,我们提出了一种用于OVLA望远镜的凹形自适应二次透镜的研究。作为初步结果,我们提出了一种具有可变厚度分布的散焦自适应校正器。定义了使用条件并评估了性能!! 13

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