Effect of Panel Misalignment Error Distribution on the Radiation Pattern of Leighton Chajnantor Telescope’s Antenna

IF 3.3 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of the Pacific Pub Date : 2024-06-01 DOI:10.1088/1538-3873/ad5047
Jia You, Zheng Wang, Rodrigo Andrés Reeves Díaz
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Abstract

The Leighton dish formerly at the Caltech Submillimeter Observatory will be reassembled to become the Leighton Chajnantor Telescope (LCT). It will be required to demonstrate high surface accuracy and controlled radiation patterns at high frequency, which are largely limited by surface error due to panel misalignment on the primary reflector. Not only the surface rms error but also the error distribution has effect on the radiation pattern of the antenna. Therefore, analyzing the effect of error distributions resulting from various panel misalignments on the radiation pattern of the antenna will facilitate better compensation of surface errors during the reassembly process. To acquire the radiation pattern of LCT’s antenna with panel misalignments, we first propose a simulation method based on physical optics and the physical theory of diffraction, which offers precise results but is time-consuming, especially at high frequencies. Then, we propose a rapid computation method that combines the method of calculating the optical path difference (OPD), the OPD fitting method, and the aperture integration method for segmented reflectors. Experimental results demonstrate that the rapid computation method is highly efficient and accurate compared to the simulation method. In order to show the effect of error distributions due to two typical panel misalignments (i.e., piston and tip-tilt) on radiation patterns, experiments are conducted using the two proposed methods for various error distributions. These experiments indicate that for the same surface rms error, smaller panel errors at smaller normalized aperture radii are more conducive to achieving improved characteristics of the radiation patterns, such as reduced peak gain losses and lower sidelobe levels. Additionally, comparison experiments also reveal that variations in piston error have a greater impact on the radiation patterns than variations in tip-tilt error under the same surface rms error.
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面板不对准误差分布对莱顿-恰南托尔望远镜天线辐射模式的影响
以前在加州理工学院亚毫米波天文台的莱顿碟形望远镜将被重新组装,成为莱顿-查南特望远镜(LCT)。它将被要求在高频率下展示高表面精度和受控辐射模式,而这在很大程度上受到主反射镜上面板错位造成的表面误差的限制。不仅表面均方根误差,误差分布也会对天线的辐射模式产生影响。因此,分析各种面板错位造成的误差分布对天线辐射模式的影响,将有助于在重新组装过程中更好地补偿表面误差。为了获得 LCT 天线在面板错位情况下的辐射模式,我们首先提出了一种基于物理光学和物理衍射理论的模拟方法,该方法可提供精确的结果,但耗时较长,尤其是在高频情况下。然后,我们提出了一种快速计算方法,该方法结合了光路差计算方法、光路差拟合方法和分段反射器的孔径积分方法。实验结果表明,与模拟方法相比,快速计算方法高效、准确。为了显示两种典型的面板错位(即活塞和尖端倾斜)造成的误差分布对辐射模式的影响,我们使用两种建议的方法对不同的误差分布进行了实验。这些实验表明,对于相同的表面均方根误差,在较小的归一化孔径半径下,较小的面板误差更有利于获得更好的辐射模式特性,如降低峰值增益损失和较低的侧叶水平。此外,对比实验还表明,在相同的表面均方根误差下,活塞误差的变化比尖端倾斜误差的变化对辐射模式的影响更大。
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来源期刊
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific 地学天文-天文与天体物理
CiteScore
6.70
自引率
5.70%
发文量
103
审稿时长
4-8 weeks
期刊介绍: The Publications of the Astronomical Society of the Pacific (PASP), the technical journal of the Astronomical Society of the Pacific (ASP), has been published regularly since 1889, and is an integral part of the ASP''s mission to advance the science of astronomy and disseminate astronomical information. The journal provides an outlet for astronomical results of a scientific nature and serves to keep readers in touch with current astronomical research. It contains refereed research and instrumentation articles, invited and contributed reviews, tutorials, and dissertation summaries.
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