Next generation millimeter-wave radar for safe planetary landing

B. Pollard, G. Sadowy
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引用次数: 30

Abstract

Safe, precise landing on planetary bodies requires knowledge of altitude and velocity, and may require active detection and avoidance of hazardous terrain. Radar offers a superior solution to both problems due to its ability to operate at any time of day, through dust and engine plumes, and ability to detect velocity coherently. While previous efforts have focused on providing near term solutions to the safe landing problem, we are designing radar velocimeters and radar imagers for missions beyond the next decade. In this paper we identify the fundamental issues within each approach, at arrive at strawman sensor designs at a center frequency at or around 160 GHz (G-band). We find that a G-band radar velocimeter design is capable of sub-10 cm/s accuracy, and a G-band imager is capable of sub-0.5 degree resolution over a 28 degree field of view. From those designs, we arrive at the key technology requirements for the development of power and low noise amplifiers, signal distribution methods, and antenna arrays that enable the construction of these next generation sensors
下一代毫米波雷达,用于安全登陆行星
安全、精确地在行星体上着陆需要了解高度和速度,可能还需要主动探测和避开危险地形。雷达为这两个问题提供了一个优越的解决方案,因为它能够在一天中的任何时间运行,穿透灰尘和发动机羽流,并且能够同步检测速度。虽然以前的努力集中在为安全着陆问题提供短期解决方案,但我们正在为下一个十年以后的任务设计雷达测速仪和雷达成像仪。在本文中,我们确定了每种方法中的基本问题,以达到中心频率在160 GHz (g波段)左右的稻草人传感器设计。我们发现,g波段雷达测速仪设计能够达到低于10厘米/秒的精度,g波段成像仪能够在28度视场内达到低于0.5度的分辨率。从这些设计中,我们得出了开发功率和低噪声放大器、信号分配方法和天线阵列的关键技术要求,这些技术要求使这些下一代传感器的构建成为可能
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