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

机译:更换高架结构以升级干草堆37米射电望远镜

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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:麻省理工学院的37米射电望远镜干草堆建于1960年代初期。在当时被认为是高性能天线时,Haystack产生了许多杰出的科学成果。最初设计为在8-10 GHz下工作的天线在不同时间进行了升级,特别是在1993年,增加了可变形的副反射器以允许在115 GHz下工作。现在正在计划进行一次重大升级,以替换现有的轭铁和塔架上支撑的整个立面结构。新天线应能够在高达325 GHz的频率下运行。在本文中,我们将描述原始设计的局限性,先前升级中使用的解决方案,以及汲取的经验教训如何导致计划中升级中使用的方法。限制现有望远镜进一步升级的主要问题是仰角结构。这些因素包括反光板的制造公差和重力下垂,支撑反光板的环形板的热滞后,高程轴承和剪切销处滑动接头的不可重复性以及钢叉和铝背架的相互作用。

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