典型月面环境下500 MHz与23 GHz频率通信信道特性研究

      Channel characterization for typical lunar environment communication at500 MHz and 23 GHz

      • 摘要: 准确掌握月面信道特性对于月球探测任务的顺利进行和科学数据的准确传输具有重大意义。该文模拟月球南极沙克尔顿撞击坑附近真实的月面环境,构建月球模拟基地、撞击坑和月球探测车等环境模型,并基于射线追踪(ray tracing, RT)法对不同频率(500 MHz和23 GHz)下无线信道进行详细的仿真分析。通过对比分析路径损耗、阴影衰落因子、莱斯K因子、均方根时延扩展和角度扩展等信道参数,揭示月面特定环境下通信信道的关键特性,丰富月表通信信道的理论认知。

         

        Abstract: Accurate mastery of the lunar surface channel characteristics is crucial for the smooth progress of lunar exploration missions and the precise transmission of scientific data. In this paper, a realistic lunar environment near Shackleton Crater at the lunar South Pole is simulated, and environmental models such as a lunar simulation base, craters, and lunar exploration vehicles are constructed. Detailed simulations and discussions of wireless channels at different frequencies (500 MHz and 23 GHz) are conducted based on the ray-tracing method. By comparing and analyzing channel parameters, such as path loss, shadow fading factor, Rician K-factor, root mean square delay spread, and angular spread, the critical characteristics of communication channels in specific lunar environments are revealed, enriching the theoretical understanding of lunar surface communication channels.

         

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