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丽江2.4米光学望远镜的视宁度研究
其他题名Research on Seeing at Lijiang 2.4m optical telescope
王德清
学位类型硕士
导师范玉峰
2019-07-01
学位授予单位中国科学院大学
学位授予地点北京
学位专业天文技术与方法
关键词视宁度 丽江2.4米光学望远镜 圆顶视宁度 微温脉动仪 侧窗控制
摘要本文分析了天文选址与实测领域中最大的影响因素——视宁度,分析了其成因、影响因素、分类、测量方法等,并具体到丽江2.4米光学望远镜:因台址优良的视宁度、大气消光、夜天光等条件,丽江2.4米光学望远镜成为我国现阶段重要的实测天文研究平台。即便台址视宁度较为优越,但圆顶结构以及内部望远镜电子设备也会引起圆顶及主镜周围温度的变化,即圆顶视宁度会引起最终视宁度的退化。考虑到本地优良视宁度的保持,配备了用于改善圆顶视宁度如侧窗、风机等一系列硬件措施,但圆顶视宁度引起的退化以及改善措施的效果没有长期定量测量过。同时观测策略如高度角、中心波长、焦距等的选择会产生不同的半峰全宽(FWHM)结果,导致望远镜的像质、实测效率都会受到影响。在站址条件、望远镜性能、终端仪器集成等都已基本确定的条件下,圆顶视宁度的改善措施以及观测策略将影响到最终的视宁度水平。本文基于STM32的嵌入式采集和RS485组网的微温脉动仪的设计,搭建了圆顶视宁度实时测量系统,通过大气参数的直接测量构建出圆顶温度场;与台站差分像视宁度监测仪(DIMM)的对比,实时反馈侧窗风机等措施的改善结果。现有的大面积圆顶侧窗作为丽江2.4米望远镜改善圆顶视宁度的最主要措施,是手动控制的,开关过程中人员走动及停留会带来额外的湍流,更会损失宝贵的观测时间,因此将侧窗进行自动化改造,使其起到减小风振及改善圆顶视宁度的作用,并能根据圆顶视宁度及外部气象条件快速准确的响应。通过DIMM、微温、望远镜FWHM数据比对,分析了各种测量方法得到的视宁度差异。通过对丽江2.4米光学望远镜的视宁度研究,为圆顶视宁度的改善以及实测效率的提高提供一些借鉴。
其他摘要Seeing, as one of the most important parameter for observatory selection and astronomical observation, is processed comprehensively and deeply by researchers. Because of the good astronomical condition including good Seeing, low atmospheric extinction and low night luminosity at the Lijiang observatory, the Lijiang 2.4m optical telescope was becoming an important platform for astronomical research in China.Dome structure and inner telescope’s instruments will bring local turbulence in the surrounding of the mirror. This effect is called Dome Seeing and it will lead to image degradation. Considering the good local Seeing condition, Windows-Blinds and other hardware were built, but Dome Seeing were not measured for long-term. As well as observing strategy like central wavelength, altitude, focus choice, Dome Seeing will affect the measured FWHM in the terminal, and it will also affect the high-resolution imaging and measuring efficiency. Under the certain condition of observatory, telescope behavior and the instrument integration, Dome Seeing and observing strategy will affect the final Seeing.Based on the embedded STM32 system and RS485 network, Micro-Thermometry is designed to measure the atmosphere parameter directly called structure constant of the refractive index (CN2), which can calculate the seeing through its path integrals. On the other hand, the old manually-operated Windows-Blinds of dome are transformed. Because manipulating the Windows-Blinds will not only bring the new turbulence and will also cost the valuable observation time. After the transformation, it can be controlled more automatically and accurately based on the Dome Seeing value and outer weather condition. All those measure are used to reduce the wind vibration and the dome seeing’s affect at the Lijiang 2.4m telescope. The different Seeing data are contracted with DIMM, Micro-Thermometry and FWHM methods to analyze the influence factors .The research of Seeing at the Lijiang 2.4m telescope in this article, can provide some constructive suggestions for Seeing improving and astronomical observation.
学科领域天文学 ; 天体物理学 ; 实测天体物理学
学科门类理学 ; 理学::天文学
页数65
语种中文
文献类型学位论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25434
专题南方基地
作者单位中国科学院云南天文台
第一作者单位中国科学院云南天文台
推荐引用方式
GB/T 7714
王德清. 丽江2.4米光学望远镜的视宁度研究[D]. 北京. 中国科学院大学,2019.
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