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ELT dome and telescope: a unique prototype in a highly seismic context

机译:埃尔特圆顶和望远镜:在高度地震背景下是一种独特的原型

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The European Extremely Large Telescope (E-ELT), with its primary mirror diameter of 39 meters, will be the largest optical/near-infrared telescope in the world and will allow scientists to investigate important unsolved issues of the universe.The dome and telescope (DMS) are designed to ensure high performance in one of the most seismic active areas in the world, Cerro Armazones in Chile.The Dome diameter is 86 m and sits on the top of a stiff concrete pier, which has been designed with horizontal seismic devices to reduce the seismic accelerations on the structures. The isolation system consists of a combination of High Damping Rubber Bearings (HDRBs) and lubricated spherical bearings.The Telescope structure has been designed to be adaptive, during operation it is extremely stiff with low damping to guarantee the pointing and tracking (fixed condition) and when subjected to strong earthquakes it is flexible with high damping (isolated condition) to reduce the accelerations on the mirrors and instruments.To fulfill these requirements, a 3D adaptive seismic isolation system has been designed with unique features. The telescope natural frequencies and damping change suddenly when the telescope is subjected to a 1-year return period seismic event, which is the maximum threshold acceleration acceptable without isolation. In the isolated configuration, the telescope frequencies range between 0.3 Hz (isolation frequency) and 30 Hz (highest frequency of interest), while in the fixed configurations the frequencies range between 2.6 Hz and 30Hz.The vertical and horizontal acceleration reduction is obtained with special devices designed for this type of applications.This paper presents the design and shows the results of the sophisticated nonlinear time history analyses performed on the DMS. The large finite element models consist of about 75000 nodes and over 110000 elements and include nonlinear spring damper elements calibrated experimentally to model the vertical and horizontal behavior of the seismic devices.
机译:欧洲极大的望远镜(E-ELT),其主要镜面直径为39米,将是世界上最大的光学/近红外望远镜,并将允许科学家调查宇宙的重要未解决的问题。圆顶和望远镜(DMS)旨在确保智利塞罗武器架构中的世界上最震动的活性地区之一的高性能。圆顶直径为86米,坐落在一个坚硬的混凝土码头的顶部,这是用横向地震设计的减少结构上的地震加速度的装置。隔离系统由高阻尼橡胶轴承(HDRB)和润滑球形轴承的组合组成。望远镜结构一直设计为自适应,在操作过程中,低阻尼非常僵硬,以保证指向和跟踪(固定条件)和当受到强烈的地震时,它具有高阻尼(隔离状态)的灵活性,以减少镜子和仪器上的加速度。为了满足这些要求,3D自适应地震隔离系统采用独特的功能设计。当望远镜受到1年返回期地震事件时,望远镜自然频率和阻尼变化,这是无隔离的最大阈值加速度。在隔离配置中,望远镜频率范围为0.3Hz(隔离频率)和30Hz(最高频率),而在固定配置中,频率范围在2.6Hz和30Hz之间。垂直和水平加速度减少,用特殊该纸张设计的设备专为这种应用而设计。本文介绍了设计,并显示了在DMS上执行的复杂非线性时间历史分析的结果。大型有限元型号由大约75000个节点组成,超过110000个元件,包括实验校准的非线性弹簧阻尼元件以模拟地震装置的垂直和水平行为。

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