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Laboratory Characterization of a Large Format, Contactless Active Mirror with Intrinsic Rejection of Vibrations

Space Telescopes and Instrumentation 2022 Optical, Infrared, and Millimeter Wave(2022)

INAF Osservatorio Astrofis Arcetri | INAF Osservatorio Astron Merate | INAF Osservatorio Astron Padova | INAF Osservatorio Astron Roma | Univ Verona | ADS Int | Microgate | ESA ESTEC

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Abstract
Large format deformable mirrors have been proposed in the last few years as key elements to implement active wave front correction for future space telescopes. Active optics is, in fact, an enabling technology for high stability, high contrast and high resolution systems. We present in this work a 40 cm diameter prototype, together with its laboratory characterization, based on voice-coil actuators. When the mirror is operated, such contact-less actuation allows the optical surface to float at a given distance from its support and the mirror is virtually decoupled from the mechanics; such condition offers an intrinsic isolation from external vibrations with no need for further damping devices. We demonstrated experimentally this concept in the laboratory on a dedicated interferometric setup, registering a substantial rejection of the vibrations injected. We will present in this work the test results and a roadmap for future developments.
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Key words
LUVOIR,space telescopes,active primary,segmented telescope,active optics,correction chain
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要点】:本文介绍了一种直径为40厘米的大型接触式主动镜,其通过内置振动抑制功能,无需额外阻尼设备,有效实现了对振动的隔离,为未来空间望远镜的主动波前校正提供了关键支持。

方法】:作者采用基于音圈驱动器的实验室表征方法,通过接触式驱动使得镜面在特定距离上浮动,实现与机械结构的虚拟解耦,从而内嵌振动隔离效果。

实验】:在专门的干涉测量装置上进行了实验验证,使用的数据集为实验中记录的振动抑制结果,实验表明该原型镜能有效抑制外部振动。