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稻城太阳射电望远镜(DSRT)天线遮挡效应仿真
引用本文:路光, 王冰, 陈耀, 吴季, 阎敬业, 武昭, 严发宝, 武林. 稻城太阳射电望远镜(DSRT)天线遮挡效应仿真[J]. 空间科学学报, 2022, 42(2): 294-305. doi: 10.11728/cjss2022.02.210202017
作者姓名:路光  王冰  陈耀  吴季  阎敬业  武昭  严发宝  武林
作者单位:山东大学空间科学研究院 威海 264209;中国科学院国家空间科学中心 北京 100190;中国科学院大学 北京 100049;中国科学院国家空间科学中心 北京 100190;空间天气学国家重点实验室 北京 100190;中国科学院大学 北京 100049
基金项目:国家重大科技基础设施子午工程项目和中国科学院前沿科学重点研究项目(QYZDY-SSW-JSC014)共同资助
摘    要:
稻城太阳射电望远镜(DSRT)由313面6 m直径抛物面天线组成。天线接收信号幅值和相位的精确修正是决定DSRT成像质量的关键因素。然而DSRT阵列可能会出现邻近天线相互遮挡的问题,从而改变接收信号的幅值和相位,影响其成像质量。利用电磁仿真软件计算了接收频率为300 MHz(波长λ=1 m)时的相邻两单元与相邻三单元两种情况。三元系统中遮挡效应的影响仅比双元系统中相关影响略为显著。在本文考虑的最严重的遮挡情况(天线边缘的投影间距D = –1λ)下,对于双/三元系统,相对于单天线系统水平和垂直增益分别降低了0.6/0.6 dB和 0.3/0.4 dB,相位偏差分别为–3.3º/–3.871º和–1.744º/–2.244º。此外还分析了其他遮挡情况。研究表明DSRT系统中的天线遮挡效应分析可由双元系统充分描述,在后期数据处理时应适当考虑该效应,尽量提升DSRT数据的利用效率和成图质量。

关 键 词:子午工程二期  稻城太阳射电望远镜  遮挡效应  幅值  相位
收稿时间:2021-02-02
修稿时间:2021-10-29

Simulations of the Antenna-shielding Effect of the Daocheng Solar Radio Telescope (DSRT)
LU Guang, WANG Bing, CHEN Yao, WU Ji, YAN Jingye, WU Zhao, YAN Fabao, WU Lin. Simulations of the Antenna-shielding Effect of the Daocheng Solar Radio Telescope (DSRT) (in Chinese). Chinese Journal of Space Science, 2022, 42(2): 294-305. DOI: 10.11728/cjss2022.02.210202017
Authors:LU Guang  WANG Bing  CHEN Yao  WU Ji  YAN Jingye  WU Zhao  YAN Fabao  WU Lin
Affiliation:1. Institute of Space Sciences, Shandong University, Weihai 264209;;2. National Space Science Center, Chinese Academy of Sciences, Beijing 100190;;3. State Key Laboratory of Space Weather, Beijing 100190;;4. University of Chinese Academy of Sciences, Beijing 100049
Abstract:
The Daocheng Solar Radio Telescope (DSRT) is a next-generation solar radio telescope funded by the Chinese Meridian Project–Phase II. DSRT is composed of 313 parabolic antennas with a diameter of six meters. The antennas are evenly distributed in a circle with a diameter of one kilometer. With the synthetic aperture imaging techniques, key factors determining the DSRT imaging quality are accurate calibrations of amplitude and phase of the received signals. Yet, under some circumstances, adjacent antennas of DSRT may shield each other, which will affects the amplitude and phase of the received signals and thus deteriorate imaging quality. In this study, such shielding effects of three- or two-antenna using the electromagnetic simulation software at frequencies of 300 MHz (λ=1 m) were simulated. The shielding effect in the three-antenna system is slightly worse than that in the two-antenna system. When the projected distance of adjacent antennas is taken to be –1λ, i.e., the most serious effect of shielding considered here, the horizontal and vertical gains of the system with two/three antennas decline by 0.6/0.6 dB and 0.3/0.4 dB, respectively, and the horizontal and vertical phase deviations are –3.3º/–3.871º and –1.744º/–2.244º, respectively, compared to the system with one antenna. Other situations with different projected shielding distances are also investigated. The results show that the two-antenna system can sufficiently describe the shielding effect associated with DSRT. Such effect should be properly taken into account when processing the future DSRT data so as to improve the data usage efficiency and imaging quality.
Keywords:Meridional project-phase II  Daocheng Solar Radio Telescope (DSRT)  Shielding effects  Amplitude  Phase
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