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2025, 05, v.42 13-18
VGOS望远镜系统稳定性设计与分析
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DOI: 10.16191/j.cnki.hbkx.2025.05.007
摘要:

甚长基线干涉测量(VLBI)系统具有超高空间分辨率和定位精度,其关键技术研发已成为各国重点关注方向。为满足当前科学研究对VLBI技术的高要求,本文研制了一套高精度的望远镜系统,可应用于甚长基线干涉测量全球观测站(VGOS)。研究重点分析了望远镜座架和反射体系统的稳定性,并对二者的精度进行了仿真分析。提出了在望远镜运行过程中使用激光跟踪仪测试座架参考点稳定性的方案,实现了对参考点位移的实时测量;利用数字摄影测量技术完成了反射体的精度测试。测试结果表明,系统各项指标均满足VGOS系统要求,该系统可应用于天文和大地测量。

Abstract:

The Very Long Baseline Interferometry(VLBI)system is characterized by its ultra-high spatial resolution and positioning accuracy,making the development of its key technologies a global priority.To meet the demanding requirements of modern scientific research utilizing VLBI,a high-precision telescope system was developed in this study,which can be applied to the VLBI Global Observing System(VGOS).The stability of the telescope mount and reflector system was analyzed,and their accuracy was evaluated through simulation.A scheme was designed to test the stability of reference points using a laser tracker during the telescope operation,achieving real-time displacement measurement of reference points.Additionally,digital photogrammetry was employed to evaluate the accuracy of the reflector.The results demonstrated that all key performance indicators met the VGOS requirements,confirming the system′s applicability in astronomical and geodetic surveys.

参考文献

[1]孙中苗,范昊鹏.VLBI全球观测系统(VGOS)研究进展[J].测绘学报,2017,46(10):1346-1353.

[2] NIELL A,WHITNEY A,PETRACHENKO B,et al.VLBI2010:current and future requirements for geodetic VLBI systems,report of working group 3to the IVS directing board[Z].Engineering,Geography,Computer Science,2005.

[3] SCHUH H,BEHREND D.VLBI:A fascinating technique for geodesy and astrometry[J].Journal of Geodynamics,2012,61:68-80.

[4] SCHUH H.Geodetic and astrometric very long baseline interferometry the IVS and its future perspectives[R].Espoo,Finland:Helmholta Association,2013.

[5] TITOV O.VLBI2020:from reality to vision[C]//VLBI2020:From Reality to Vision,IVS 2010General Meeting Proceedings.Hobart:IVS,2010:60-64.

[6] HASE H,BEHREND D,MA C,et al.The emerging VGOS network of the IVS[C]//The Emerging VGOS Network of the IVS,IVS 2012General Meeting Proceedings.Spain:IVS,2012:8-12.

[7] PETRACHENKO B,NIELL A,BEHREND D,et al.Design aspects of the VLBI2010system[R].Greenbelt:National Aeronautics and Space Administration,2009.

[8]李金岭,王广利.上海VLBI站相对于欧亚板块稳定区域的运动[J].中国科学院上海天文台年刊,2001(22):57-62.

[9]洪晓瑜.VLBI技术的发展和“嫦娥工程”中的应用[J].自然杂志,2007,29(5):297-299.

[10]项英,张秀忠.VLBI技术新进展[J].天文学进展,2003,21(3):185-194.

[11]程景全.天文望远镜原理和设计[M].南京:南京大学出版社,2020.

[12]段宝岩,苏玉鑫,仇原鹰,等.新一代大射电望远镜机电光一体化设计研究[J].中国机械工程,1999,10(9):1002-1004.

[13]左营喜,李阳,孙继先,等.德令哈13.7m望远镜重力变形研究[J].天文学报,2011,52(2):152-159.

[14]范钦红,范生宏,左营喜,等.基于数字摄影测量技术的13.7 m毫米波天线面形检测[J].天文学报,2010,51(2):210-216.

[15]宋世泽,王广利,郑勇,等.基于自动实时监测系统的天马VGOS望远镜热膨胀研究[J].天文学进展,2022,40(3):466-476.

[16]BAARS J W M.Design features of some radio telescopes[M].New York,NY:Springer,2007:201-245.

[17]VON HOERNER S,WONG W Y.Gravitational deformation and astigmatism of tiltable radio telescopes[J].IEEE Transactions on Antennas and Propagation,1975,23(5):689-695.

基本信息:

DOI:10.16191/j.cnki.hbkx.2025.05.007

中图分类号:P111.44

引用信息:

[1]张强,王大为.VGOS望远镜系统稳定性设计与分析[J].河北省科学院学报,2025,42(05):13-18.DOI:10.16191/j.cnki.hbkx.2025.05.007.

基金信息:

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