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The 3,5m all SiC Telescope for SPICA

机译:35米的所有SiC望远镜为Spica

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摘要

Placed on the L2 Lagrangian point, the Space Infrared Telescope for Cosmology and Astrophysics (SPICA) will operate in the 5 to 200 μm wavelength range, at 4.5K. The large aperture telescope (3.5m diameter in a single piece) requires a strong manufacturing mastering, associated with high technical performances. The background acquired by EADS-Astrium (France) on the 3.5m Silicone Carbide Herschel Telescope is a key for the success of the SPICA development. EADS-Astrium has been awarded by the Japan Aerospace Exploration Agency (JAXA) and Sumitomo Heavy Industries to assess the feasibility of the 3.5m all SiC telescope through a design phase contract. The Telescope driving requirements are the large diameter of 3.5m especially critical for the manufacturing aspects, and the Wave Front Error which has to be kept below 350nm rms over a large temperature range from ambient to the operational temperature of 4.5K which requires a strong mastering of the distortions.
机译:放置在L2拉格朗日点,宇宙学和天体物理学(SPICA)的空间红外望远镜将在5至200μm波长范围内运行,在4.5k。大型孔径望远镜(单件中的3.5米直径)需要强大的制造母版,与高技能表现相关。 EADS-Astrium(法国)在3.5米硅树脂碳化渣拍摄望远镜所获得的背景是Spica开发成功的关键。 EADS-Astrium已被日本航空航天勘探机构(JAXA)和Sumitomo Report Industress颁发的,以评估3.5M所有SIC望远镜通过设计阶段合同的可行性。望远镜驾驶要求的直径为3.5米,特别适用于制造方面,并且波前误差在大型温度范围内的450℃下方的波前误差为4.5K的操作温度,这需要强大的掌握扭曲。

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