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Experimental Study of Breakaway System for the Fast-steering Secondary Mirror Prototype of the GMT

机译:GMT快速转向副镜原型分离系统的实验研究

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The Fast-steering Secondary Mirror (FSM) of Giant Magellan Telescope (GMT) consists of seven 1.1 m diameter circular segments with an effective diameter of 3.2 m. which are conjugated 1:1 to the seven 8.4 m segments of the primary. Each FSM segment contains a tip-tilt capability for fast guiding to attenuate telescope wind shake and mount control jitter by adapting axial support actuators. Breakaway System (BAS) is installed for protecting FSM from seismic overload or other unknown shocks in the axial support. When an earthquake or other unknown shocks come in. the springs in the BAS should limit the force along the axial support axis not to damage the mirror. We tested a single BAS in the lab by changing the input force to the BAS in a resolution of 10 N and measuring the displacement of the system. In this paper, we present experimental results from changing the input force gradually. We will discuss the detailed characteristics of the BAS in this report.
机译:巨型麦哲伦望远镜(GMT)的快速转向辅助镜(FSM)由七个直径为1.1 m的圆形部分组成,有效直径为3.2 m。 1:1与七个主要8.4 m片段共轭。每个FSM段均具有倾斜功能,可通过调整轴向支撑致动器来快速引导,以减弱望远镜的风振并安装控制抖动。安装了脱离系统(BAS),用于保护FSM免受地震过载或轴向支撑件中的其他未知冲击的影响。当发生地震或其他未知冲击时,BAS中的弹簧应限制沿轴向支撑轴的力,以免损坏后视镜。我们在实验室中通过以10 N的分辨率更改对BAS的输入力并测量系统的位移来测试单个BAS。在本文中,我们介绍了逐渐改变输入力的实验结果。我们将在本报告中讨论BAS的详细特征。

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