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Replacement of Elevation Structure to Upgrade Haystack 37-m Radio Telescope

机译:更换高程结构升级Haystack 37-M射频望远镜

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Haystack, MIT's 37-m radio telescope, was built in the early 1960s. At the time considered to be a high-performance antenna, Haystack produced a number of outstanding scientific results. The antenna, originally designed to operate at 8-10 GHz, was upgraded at various times, notably in 1993 with the addition of a deformable subreflector to allow operations at 115 GHz. Planning is now underway for a major upgrade with the replacement of the entire elevation structure that is supported on the existing yoke and tower. The new antenna should be capable of operating at up to 325 GHz. In this paper, we will describe the limitations of the original design, the solutions used in the previous upgrades, and how the lessons learned led to the approach used in the planned upgrade. The major issues limiting the further upgrade of the existing telescope were in the elevation structure; these included fabrication tolerances and gravity sag of the reflector panels, thermal lag of a ring plate supporting the reflector panels, non-repeatable behavior of the sliding joint at the elevation bearing and shear pins, and the interaction of the steel yoke and the aluminum backstructure.
机译:MIT的37-M射频望远镜大海捞,建于20世纪60年代初。当时被认为是高性能天线,干草堆产生了许多优秀的科学结果。最初设计用于8-10 GHz的天线在不同时间升级,特别是在1993年,添加可变形的子折叠器,以允许在115 GHz下进行操作。现在正在进行规划,替代现有磁轭和塔楼支持的整个高程结构进行了重大升级。新天线应能够在高达325 GHz上运行。在本文中,我们将描述原始设计的局限性,在先前升级中使用的解决方案,以及如何学习的经验教训导致计划升级中使用的方法。限制现有望远镜进一步升级的主要问题在仰角结构;这些包括反射器板的制造公差和重力凹陷,环形板的热滞后支撑反射器板,在升降轴承和剪切销处的滑动接头的不可重复行为,以及钢轭和铝制背部的相互作用。

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