用户名: 密码: 验证码:
平均风作用对天马望远镜面形精度和指指向精度的影响
详细信息    查看全文 | 推荐本文 |
  • 英文篇名:The Effect of Mean Wind Power on Antenna Surface Accuracy and Pointing Accuracy of the Tian Ma Telescope
  • 作者:付丽 ; 王宇飞 ; 钱宏亮
  • 英文作者:FU Li;WANG Yu-fei;QIAN Hong-liang;Shanghai Astronomical Observatory, Chinese Academy of Sciences;Harbin Institute of technology;
  • 关键词:天线结构 ; 风荷载 ; 面形精度 ; 指向精度
  • 英文关键词:antenna structure;;wind load;;surface accuracy;;pointing accuracy
  • 中文刊名:TWJZ
  • 英文刊名:Progress in Astronomy
  • 机构:中国科学院上海天文台;哈尔滨工业大学(威海)土木工程系;
  • 出版日期:2019-06-15
  • 出版单位:天文学进展
  • 年:2019
  • 期:v.37
  • 基金:国家自然科学基金(51678191,U1631114,11873015,11203062);; 国家重点研发计划(2018YFA0404702)
  • 语种:中文;
  • 页:TWJZ201902006
  • 页数:16
  • CN:02
  • ISSN:31-1340/P
  • 分类号:79-94
摘要
天马望远镜的最高工作频段为43 GHz。为保证高质量的观测结果,需要研究风载荷对天线精度的影响。首先对观测站实测的风速风向数据做了统计分析,结果显示:10 m高度处10min时距平均风速小于4 m·s~(-1)的占比超过80%,主导风向为北-西北方向。然后,通过将倾斜仪实测结果与有限元模拟结果进行对比,验证了模拟的有效性,并进一步分析了在不同迎风姿态、不同风速下天线结构的平均风荷载响应,以及天线面形精度和指向精度的变化。结果表明,平均风荷载对天线指向精度,尤其是俯仰角指向精度的影响较大,对面形精度的影响较小;在弹性范围内,天线面形精度和指向精度与风速间均为二次关系。研究结果可为天线面形精度和指向精度的评估提供参考。
        The highest working frequency band of the Tian Ma Telescope(TM65 m) is 43 GHz. To ensure high-quality observations, it is necessary to study the influence of wind load on the antenna accuracy. Firstly, the wind speed and direction data measured at the observation station were statistically analyzed. The results show that the wind speed below 4 m · s-1 account for more than 80% of the wind speed at 10 m height, and the dominant wind direction is north-northwest. Then, by comparing the measured data of the inclinometer and the finite element simulation results, the effectiveness of the simulation is verified. Furthermore,the average wind load response of the antenna structure under different windward attitudes and different wind speeds is analyzed, as well as the antenna surface accuracy and pointing accuracy. The results show that the average wind load has a greater influence on the pointing accuracy of the antenna, in particular the pitching pointing accuracy, and has little effect on the accuracy of the surface shape; within the elastic range, the relationship between the antenna surface shape accuracy and the wind speed is a quadratic relationship, so is pointing accuracy and wind speed's relationship. These results can provide reference for the evaluation of antenna surface accuracy and pointing accuracy.
引文
[1]刘国玺,郑元鹏.上海65米射电望远镜天线方案设计报告[R].石家庄:中国电子科技集团公司第五十四研究所, 2009:5
    [2]叶尚辉,李在贵.天线结构设计[M].西安:西北电讯工程学院出版社, 1986:98
    [3]刘岩,钱宏亮,范峰.大型射电望远镜结构风荷载特性研究[J].红外与激光工程, 2015, 44(01):148
    [4]王春圆.巨型射电望远镜风荷载特性的数值模拟研究.硕士论文.哈尔滨:哈尔滨工业大学, 2012:19
    [5]赵彦.大射电望远镜指向误差建模分析与设计研究.博士论文.西安:西安电子科技大学, 2008:27
    [6]虞梦月. 110米口径超大型全可动天线轴系误差对指向精度的影响.硕士论文.西安:西安电子科技大学, 2014:9
    [7]李素兰.超大型全可动反射面天线高指向精度关键技术研究.博士论文.西安电子科技大学, 2014:39
    [8] Angeli G Z, Cho M K, Sheehan M, et al. Characterization of Wind Loading of Telescopes, Proc. SPIE,Integrated Modelingvof Telescopes, 2002, 4757:72
    [9] Gawronski W. Modeling wind-gust disturbances for the analysis of antenna pointing accuracy[J]. Antennas&Propagation Magazine IEEE, 2004, 46(1):50
    [10] Gawronski W. Control and pointing challenges of antennas and telescopes[C] American Control Conference,2005. Proceedings of the. IEEE, 2005, 6:3758
    [11]吕明华,闫江雨,姚仁太,等.风向的统计方法研究[J].气象与环境学报, 2012, 28(03):83
    [12]范峰,钱宏亮.上海65米射电望远镜天线结构力学分析核查报告[R].哈尔滨:哈尔滨工业大学空间结构研究中心, 2010:13
    [13]钱宏亮,刘岩,范峰,等.上海65m射电望远镜太阳辐射作用分析[J].工程力学, 2012, 29(10):378
    [14]付丽,董健,凌权宝,等.天马望远镜结构重力变形对面形和指向精度影响[J].电波科学学报, 2017, 32(3):318

© 2004-2018 中国地质图书馆版权所有 京ICP备05064691号 京公网安备11010802017129号

地址:北京市海淀区学院路29号 邮编:100083

电话:办公室:(+86 10)66554848;文献借阅、咨询服务、科技查新:66554700