首页> 外文会议>Conference on UV, Optical, and IR Space Telescopes and Instruments 29-31 March 2000 Munich, Germany >Stretched membrane with electrostatic curvature (SMEC): A new technology for ultra-lightweight space telescopes
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Stretched membrane with electrostatic curvature (SMEC): A new technology for ultra-lightweight space telescopes

机译:静电曲率拉伸膜(SMEC):超轻型太空望远镜的新技术

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Very large space telescopes with primary mirrors made of flat segments have been recently proposed.~1 The segments would be extremely lightweight, made like pellicles from stretched, reflective membranes. Here we consider the use of such membrane primary mirrors in which slight concave curvature is induced by electrostatic force, by application of a potential difference between the membrane and a control electrode behind. In this way segmented spherical or paraboloidal primaries of long focal length can be made directly, eliminating the correction optics needed when flat segments are used. The electric potential would be spatially and temporaly controlled to obtain uniform curvature despite non-uniformity in membrane tension, to create slight asphericity if needed and to provide active damping of vibrations. We report the operation of a small prototype telescope with a SMEC primary. A design for a 3.2-m space prototype is described, based on the two-mirror anastigmat of Schewartzschild~2 and Couder~3. A 400 m radius primary is combined with a single concave secondary flying in formation at a distance of 190 m. Together they form a wide-field, well-corrected focus at f/30. A larger telescope with much higher diffraction limited resolution could be made simple by adding more segments of the 27 m diameter parent primary to the formation. The TPF nulling interferomer could be made with similarly sized elements in a 100 m formation, configured as segments of a kilometer focal length parent~4. A very large SMEC telescope might be made from a continuous 10 x 1000 m membrane, rolled up for launch. Cryogenic cooling for all these configurations would be accomplished by additional spacecraft int eh formation to block direct solar illumination of the telescope elements.
机译:最近已经提出了非常大的太空望远镜,其带有由平坦部分制成的主镜。〜1这些部分非常轻巧,就像由拉伸的反射膜制成的薄膜一样。在这里,我们考虑使用这样的膜主镜,其中通过在膜和后面的控制电极之间施加电势差,由静电力引起轻微的凹曲率。通过这种方式,可以直接制作长焦距的分段球面或抛物面原色,从而消除了使用扁平段时所需的校正光学元件。尽管膜张力不均匀,但在空间和时间上都可以控制电位以获得均匀的曲率,如果需要的话可以产生轻微的非球面性,并提供主动的振动阻尼。我们报告了带有SMEC主镜的小型原型望远镜的操作。描述了一个基于Schewartzschild〜2和Couder〜3的两面镜的3.2 m空间原型的设计。半径为400 m的一次生层与一个凹入的二次生飞层在190 m处相结合。它们共同构成了f / 30的广域,校正良好的焦点。通过在地层中增加27 m直径母层的更多段,可以简化具有更大衍射极限分辨率的大型望远镜。可以用100 m地层中尺寸相似的元素制成TPF无效干扰剂,并配置为km焦距parent〜4的片段。一个非常大的SMEC望远镜可能是由连续的10 x 1000 m膜制成的,卷起来发射。所有这些配置的低温冷却将通过额外的航天器结构来完成,以阻止望远镜元件的直接太阳光照射。

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