摘要
提出了理想反射面及2参数、5参数和6参数最佳吻合抛物面方法,计算大型卡氏天线结构重力变形后主反射面板的调整量和对应的副反射面调整量,同时分析馈源偏焦对天线电性能的影响.以上海天文台天马65 m望远镜(TM65m)为研究对象,综合对比分析促动器调整量、6杆并联机构调整量、主反射面精度及偏焦后天线指向变化等,认为针对实际结构而言,经过调整修正后,6参数最佳吻合抛物面方法可以作为高精度天线理想的计算面板变形主动控制量方法,计算结果为天线的主动控制提供初调数据.
The methods of ideal reflector surface, two-parameter, five-parameter, and six-parameter best-fit paraboloid are presented in this paper. Based on these methods, the adjustment values of gravity deformations are calculated for the main reflector of large-scale Cassegrain antenna. Accordingly, the positions of subrefiector are corrected, and the effects of offset-focus on electric performance are also analyzed. Taking Shanghai 65 m antenna as a research object, the adjustment values of actuator and hexapod, the accuracy of the main reflector surface, and the pointing error after offsetting the focus are contrasted. As a result, the method of six-parameter best-fit paraboloid is ideal to calculate active control value for antenna panels after the effects of feed defocus have been adjusted and modified. The results offer data for the active control of antenna.
出处
《天文学报》
CSCD
北大核心
2015年第4期378-390,共13页
Acta Astronomica Sinica
基金
上海市科学技术委员会科研计划项目(08DZ1160100)
中国科学院知识创新工程重大项目(KJCX-YW-18)
国家自然科学基金项目(Y347201001)资助
关键词
望远镜
方法
数据分析
技术
其他诸多方面
telescopes, methods
data analysis, techniques
miscellaneous
