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A spatiotemporal analysis of the effect of ambient temperatures on the thermal behaviour of the Lunar Laser Ranging optical telescope at Hartebeesthoek Radio Astronomy Observatory

机译:环境温度对Hartebeesthoek射电天文台月球激光测距光学望远镜热行为影响的时空分析

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摘要

Development of the 1-meter aperture Lunar Laser Ranging (LLR) telescope is underway at the Hartebeesthoek Radio Astronomy Observatory (HartRAO) which is expected to achieve sub-centimeter range precision and accuracy to the Moon, for enhanced tests of Earth-Moon system dynamics. Key to the operational performance of the telescope is thermal analysis of the telescope composite structure including the optical mirrors. This study presents a thermal analysis on the integrated component materials comprising the LLR telescope in ANSYS, with the aim of simulating its thermal behaviour in response to site-based ambient air temperature (TA). Results show that for a full day TA profile spanning the time period 00:00 to 23:59 the resulting range of simulated thermal variations measured at 12:00 midday and 23:59 nighttime across the telescope composite structure was found to be 9.11 ºC to 10.03 ºC and 9.12 ºC to 9.86 ºC respectively. In particular, the spider assembly and outer tube surface had the largest range of thermal variations i.e. greater than absolute 1 ºC and thus, could be the main areas on the telescope where most thermal variations would occur. Furthermore, validation of the outer tube thermal variations using the 64 Resistant Temperature Detector (RTD) sensors mounted onto the test tube, showed relatable overall thermal variations of about 2 ºC, at wind speeds of 0 to 0.4 km/h. In overall, these findings provide a typical expectation of the LLR telescope thermal behavior in response to TA at the site; and thus could be used as a guide to develop an RTD-based thermal monitoring system for the HartRAO LLR optical telescope.
机译:Hartebeesthoek射电天文台(HartRAO)正在进行1米孔径月球激光测距(LLR)望远镜的开发,该望远镜有望实现到月球的亚厘米范围精度和精确度,以增强对月球系统动力学的测试。望远镜运行性能的关键是对包括光学镜的望远镜复合结构进行热分析。这项研究对ANSYS中包含LLR望远镜的集成部件材料进行了热分析,目的是模拟其响应基于现场环境空气温度(TA)的热行为。结果表明,对于整个时间跨度从00:00到23:59的TA分布,发现在整个望远镜复合结构中模拟的热变化的最终范围是中午12:00和夜间23:59,在整个望远镜复合结构中为9.11ºC至分别为10.03ºC和9.12ºC至9.86ºC。特别是,星形轮组件和外管表面具有最大的热变化范围,即大于绝对1ºC,因此可能是望远镜上发生最大热变化的主要区域。此外,使用安装在试管上的64个电阻温度检测器(RTD)传感器对外管的热变化进行验证,结果表明,在0至0.4 km / h的风速下,相关的整体热变化约为2ºC。总体而言,这些发现提供了对LLR望远镜响应现场TA的热行为的典型期望。因此可以用作开发基于HartRAO LLR光学望远镜的基于RTD的热监测系统的指南。

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