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作 者:Rui-Gang Wang Yan Su Zong-Yu Zhang Qing Zhang Chen-Di Liu Tian-Sheng Hong Shu-Ning Liu Wei Du Shun Dai Chun-Yu Ding Chun-Lai Li
机构地区:[1]National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China [2]School of Astronomy and Space Science,Universty of Chinese Academy of Sciences,Beijing 100049,China [3]The 54th Research Institute of China Electronics Technology Group Corporation,Shijiazhuang 050081,China [4]Institute of Moon-base Exploration and Observation,Institute of Advance Study,Shenzhen University,Shenzhen 518060,China
出 处:《Research in Astronomy and Astrophysics》2022年第10期11-23,共13页天文和天体物理学研究(英文版)
基 金:funded by the National Natural Science Foundation of China(NSFC,Grant No.12073048);supported by the Key Research Program,Chinese Academy of Sciences,Grant No.ZDBS-SSW-JS007。
摘 要:The permittivity of lunar regolith is crucial for further processing and interpretation of radar data.The conventional hyperbolic fitting method ignores the antenna height and spacing and has a significant error at a shallow depth.For the new method that considers the layout of the antenna,the influencing factors have not been studied.In this paper,we studied the influence of the position of the hyperbola peak and time zero on the new method for permittivity derivation.The simulation results show that when the input errors of time zero,abscissa and ordinate of the hyperbolic peak are±2 ns,±0.02 m and±0.2 ns respectively,the average errors of the calculated results by points within 1 m from the hyperbolic peak are 10.0%,16.7%and 38.2%,respectively.To improve the accuracy,we used the average results by points that are horizontally more than 1 m away from the hyperbola peak.Hence,we calculated the permittivity of the lunar regolith by the new method based on Lunar Penetrating Radar data.The average permittivity of the lunar regolith is estimated to be 3.3±1.2.
关 键 词:Moon-techniques radar astronomy-techniques image processing
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