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Introduction of a 2.5m telescope mount

机译:引入2.5米望远镜安装

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摘要

Telescope is a very important tool for astronomers to survey and study the stellar stars and astronomical phenomena. Theperformance of a telescope is its capability to track the observing objects and keep the image on the field of view duringthe observing period. All these functions will be achieved by telescope mount, including mount control system. Themount is to support the mirror cell and keep the mirror cell position stability. Meanwhile, with the help of control system,the mount acts as tracker of the observing objects. So, for a telescope, the mount and its control system play an importantrole during the telescope operation. This paper introduces the structure design and analysis of the mount system of a2.5m optical/infrared telescope, such as azimuth axis, elevation axis, M2 positioning system, M3 positioning system, andso on. Especially, an innovative support and escape mechanism of M3 will be proposed and analysed in this paper.
机译:望远镜是天文学家调查和研究恒星恒星和天文现象的一个非常重要的工具。望远镜的性能是其能够跟踪观察物体并将图像保持在观察期间的视野上。所有这些功能将通过望远镜安装,包括安装控制系统。 Themount是支持镜像单元并保持镜像单元位置稳定性。同时,在控制系统的帮助下,坐骑用作观察物体的跟踪器。因此,对于望远镜,安装座及其控制系统在望远镜操作期间起着重要的摩擦。本文介绍了A2.5M光/红外望远镜安装系统的结构设计和分析,如方位角轴,升降轴,M2定位系统,M3定位系统,ANSO。特别是,本文将提出和分析M3的创新支持和逃避机制。

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