Method of constructing the primary error matrix of the RT-32 radio telescope in an automated mode

Pub Date : 2021-07-01 DOI:10.15407/KNIT2021.03.066
V. Vlasenko, Kyiv Ukraine Test, V. M. Mamarev, V. V. Ozhynsky, O. Ulyanov, V. Zakharenko, M. Palamar, A. Chaikovskyi
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引用次数: 2

Abstract

2020 was the year of introduction of the Ukrainian new generation radio telescope RT-32 into the experimental operation. The test results of maser hydrogen and hydroxyl lines obtained during the experimental operation confirmed the correctness of the calculations and technological solutions of Ukrainian scientists and manufacturers Consortium. One of the further development directions of RT-32 as a radio astronomical research tool is to increase the accuracy of pointing the radio telescope to radio astronomical sources. One of the further development directions of RT-32 as a radio astronomical research tool is to increase the accuracy of pointing the radio telescope to astronomical radio sources. The latter is to be achieved by automating the processes of guidance error matrices formation and their integration during the observations. The formation of such a matrix presupposes taking into account the structural features of the antenna system and weather condition. The paper presents the results of geodetic measurements of the antenna system surface on different elevation angle, construction of the 3D model of the reflector. The method of constructing the error matrix, which at this stage of research provides the necessary simplicity of perception and interpretation of the obtained results by the human operator, is proposed. The results of the developed method verification using reference radio sources are given and the error matrices of elevation and azimuth pointing (dimension 81x81 elements) obtained with the use of said method are presented. The introduction of the results presented in the article into the radio telescope control system allowed increasing the accuracy of RT-32 radio telescope pointing in the C- and K- bands to the value of ~36″. This work partially was supported by Latvian Council of Science project "Joint Latvian-Ukrainian study of peculiar radio galaxy “Perseus A” in radio and optical bands. Nr: lzp-2020/2-0121".
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RT-32射电望远镜主误差矩阵的自动构造方法
2020年是乌克兰新一代射电望远镜RT-32进入实验运行的一年。在实验操作中获得的微波激射氢和羟基线的测试结果证实了乌克兰科学家和制造商联盟的计算和技术解决方案的正确性。RT-32作为射电天文研究工具的进一步发展方向之一是提高射电天文望远镜指向射电天文源的精度。RT-32作为射电天文研究工具的进一步发展方向之一是提高射电望远镜对天文射电源的指向精度。后者是通过在观测过程中自动生成制导误差矩阵及其积分来实现的。这种矩阵的形成以考虑天线系统的结构特征和天气条件为前提。本文介绍了天线系统表面在不同仰角下的大地测量结果,并建立了反射面三维模型。提出了一种构造误差矩阵的方法,该方法在研究阶段为人类操作员对所得结果的感知和解释提供了必要的简洁性。给出了利用参考射电源验证该方法的结果,并给出了用该方法得到的仰角指向和方位角指向(尺寸为81x81元)的误差矩阵。将本文提出的结果引入射电望远镜控制系统,可以将指向C和K波段的RT-32射电望远镜的精度提高到~36″。这项工作部分得到了拉脱维亚科学委员会项目“拉脱维亚-乌克兰联合研究无线电和光学波段的特殊射电星系“英仙座A””的支持。Nr: lzp - 2020/2 - 0121”。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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