Conversion of a Telecommunications Antenna into a Radio Telescope: Laser Scanner Measurements of Optics and Dish Surface Quality of a Cassegrain Antenna

Author:

Rasha Asif1ORCID,Natusch Tim1,Granet Christophe2,Gulyaev Sergei1

Affiliation:

1. Institute for Radio Astronomy and Space Research, Auckland University of Technology, Auckland, New Zealand

2. Lyrebird Antenna Research Pty Ltd, NSW, Australia

Abstract

A number of countries have identified redundant large telecommunications antennas (TA) and indicated their intention to convert them into radio telescopes (RT). As the efficiency of a parabolic dish radio telescope depends on its surface quality and optical alignment, a careful assessment of these properties should be undertaken before conversion. Here, as a case study, we describe a laser scanning (LS) procedure we developed and used for the Warkworth 30[Formula: see text]m Cassegrain antenna. To investigate gravity-induced mechanical deformation of the antenna surfaces and structure, we conducted measurements at elevation angles ranging from 6 to 90 degrees. The ability of a laser scanner to survey its nominal [Formula: see text] steradian surroundings allows for simultaneous study of the main and subreflectors, readily permitting a dynamic investigation of variation of the telescope optics as elevation changes occur. In particular, the method we present here allows determination of the surface quality of both main and subreflectors, the displacement between centers of the reflectors, their relative rotations and focal length variation as a function of elevation angle. We discuss details of settings, measurements, data processing and analysis focusing on possible difficulties and pitfalls. In our case study, no significant elevation-dependent surface deformation of the reflectors was observed, with the overall standard deviation of the postfit residuals varying between 1.0 and 1.7[Formula: see text]mm as elevation angle changes from 90 to 6, respectively. We, therefore, conclude that in our case both the main reflector and the subreflector, as well as the telescope optics, remain unaffected by gravitational deformation within the accuracy of the measurements, a conclusion that can possibly be extended to the similar class of TA currently considered for conversion.

Funder

Auckland University of Technology, New Zealand

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Instrumentation

Cited by 4 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Untrained single scanning phase retrieval neural network for surface deformation measurement of large-aperture antennas;Optics and Lasers in Engineering;2024-12

2. Research on laser spectrum of large-aperture antenna subreflector pose measurement;Sixth Conference on Frontiers in Optical Imaging and Technology: Imaging Detection and Target Recognition;2024-04-30

3. 大口径天线副面姿态测量技术研究进展;SCIENTIA SINICA Physica, Mechanica & Astronomica;2023-08-01

4. Electromagnetic Model of Dual Reflector Radio Telescope based on Laser Scanning Survey;2020 IEEE Microwave Theory and Techniques in Wireless Communications (MTTW);2020-10-01

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