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Instrumentation and observation target of the Lunar Radar Sounder (LRS) experiment on-board the SELENE spacecraft

机译:SELENE航天器上的月球雷达测深仪(LRS)实验的仪器和观测目标

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The Lunar Radar Sounder (LRS) on-board the SELENE lunar orbiter is currently being equipped to provide the data of subsurface stratification and tectonic features in the shallow part (several km deep) of the lunar crust, by using an FM/CW radar technique in HF (~5 MHz) frequency range. Knowledge of the subsurface structure is crucial to better understanding, not only of the geologic history of the Moon, but also of the Moon's regional and global thermal history of the Moon and of the origin of the Earth-Moon system. In addition to the subsurface radar experiment, LRS will provide the spectrum of plasma waves and solar and planetary radio waves in a wide frequency range from 10 Hz to 30 MHz. This paper provides the basic function parameter of the LRS system based on the final function test and proposes observation targets and data analysis that will provide important information leading to a greater understanding of the tectonics and thermal history of the Moon
机译:目前已装备SELENE月球轨道器上的月球雷达探测器(LRS),以使用FM / CW雷达技术提供月球地壳浅层(数千米深)的地下分层和构造特征数据在HF(〜5 MHz)频率范围内。对地下结构的了解对于更好地理解月球至关重要,不仅是对月球的地质历史的了解,而且对月球的区域性和全球性月球热史以及地月系统的起源也是如此。除了地下雷达实验,LRS还将提供从10 Hz到30 MHz的宽频率范围内的等离子波以及太阳和行星无线电波的频谱。本文基于最终功能测试提供了LRS系统的基本功能参数,并提出了观测目标和数据分析,这些数据将提供重要信息,从而使人们对月球的构造和热史有更深入的了解。

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