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Semi-kinematic mount of the FIREBALL large optics

机译:FIREBALL大型光学元件的半运动学安装

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In the context of the NASA CNES FIREBALL balloon borne experiment, we present the design of a semi-kinematic mount to hold the 1 meter class mirrors of this mission. To maintain these large optics in a reasonable mass and price budgets we choose thin ULE mirrors with a thickness over diameter ratio of 1/16. Such thin mirrors require a multi support mount to reduce self weight deflection. Classical multi support mount used for ground based telescope would not survive the level of shock observed in a balloon experiment either at parachute opening or landing. To firmly maintain these mirrors in several points without noticeably deforming them we investigated the design of a two stages semi-kinematic mount composed of 24 monopods. We present the detailed design of this innovative mirror mount, the finite element modeling with the deduced optical wavefront deformation. During the FIREBALL integration and flight campaign in July 2007 at CSBF, we confirmed the validity of the mechanical concept by obtaining an image quality well within the required specifications. Variants of this approach are potentially applicable to large thin mirrors on ground-based observatories.
机译:在NASA CNES FIREBALL气球载实验的背景下,我们提出了一种半运动支架的设计,该支架可容纳此任务的1米级镜子。为了使这些大型光学器件保持在合理的质量和价格预算范围内,我们选择厚度/直径比为1/16的薄型ULE反射镜。这种薄镜需要多支撑架,以减少自重变形。在降落伞打开或着陆的气球实验中,传统的用于地面望远镜的多支撑座无法经受住在气球实验中观察到的震动水平。为了将这些反光镜牢固地保持在几个位置上,而又不会使其明显变形,我们研究了由24个单脚架组成的两级半运动学底座的设计。我们介绍了这种创新的反射镜安装架的详细设计,以及推论出的光波前变形的有限元建模。在2007年7月于CSBF进行的FIREBALL集成和飞行活动中,我们通过获得符合要求规格的图像质量,确认了机械概念的有效性。这种方法的变体可能适用于地面天文台上的大型薄镜。

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