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地基深空探测雷达研究进展与展望

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地基深空探测雷达通过主动发射电磁波,并接收反射信号,实现对深空目标的精确测量,是研究月球、近地小行星、类地行星等深空目标的重要手段.地基深空探测雷达可以高精度测量深空目标的轨道、自转、形貌等特征,具有全天时全天候观测、精确测距、高分辨率成像等优势,对近地小行星防御和行星科学研究具有重要意义.本文介绍了地基深空探测雷达的概念内涵,梳理了地基深空探测雷达系统的国内外发展现状,回顾了地基深空探测雷达过去数十年间取得的重要历史贡献,包括月球表面高分辨率成像与永久阴影区水冰探测、近地小行星精细形貌特征获取、近地小行星轨道与自转等物理特性精确测量、近地小行星撞击防御任务处置效果快速评估、类地行星表面高分辨率成像与地质结构研究等一系列重要研究成果.在此基础上,本文介绍了分布孔径深空探测雷达的创新机理,通过多部雷达单元协同观测,可突破传统集中式体制地基深空探测雷达的口径和发射功率物理极限,形象称之为"中国复眼"雷达.最后,本文介绍了分布孔径深空探测雷达系统研制与观测实验等最新研究进展,展示了分布孔径深空探测雷达对月球二维成像和三维成像的实验结果,并对地基深空探测雷达的未来发展趋势进行了展望.
Developments and Prospects of Ground-Based Deep-Space Radar
Ground-based deep-space radar,the most powerful method for post-discovery,remote physical and dynami-cal characterization of near-Earth objects,is an important method for studying solar system celestial bodies such as the moon,near-Earth asteroids,and terrestrial planets.The advantages of ground-based deep-space radar include all-day and all-weather,accurate ranging,high-resolution imaging.Ground-based deep-space radar can obtain the physical char-acterizations including orbit,rotation,topography of the objects,prevent newly discovered objects from being lost,re-duce uncertainties on orbital elements by orders of magnitude,and greatly improving impact probability estimates com-pared to optical-only datasets,which is crucial for near-Earth asteroids defense and planetary science.The key facilities for ground-based deep-space radar are the 305-meter Arecibo Observatory(decommissioned in 2020 after two cable fail-ures)in Puerto Rico and 70-meter Goldstone Solar System Radar(GSSR)in California,which played a critical and unique role in the tracking and characterization of near-Earth objects in past decades.This paper introduces the back-ground of ground-based deep-space radar,summarizes the development status of ground-based deep-space radar sys-tem,and reviews remarkable historical contributions of ground-based deep-space radar detection,such as high-resolution imaging of the surface of the Moon,Venus,Mercury and Mars,identifications of water ice deposits in polar regions on the Moon and Mercury,precise measurements of the orbits and shapes of near-Earth asteroids,rapid assess-ment of impact effect in near-Earth asteroid defense mission.However,existing ground-based deep-space radars are cen-tralized radar systems with a single antenna,which have some inherent limitations including limited detection range and high failure rate due to the physical limits of antenna size and transmitter power.This paper introduces the innovative concept of the distributed aperture deep-space radar system,which consists of dozens of radar units.Each radar unit has separate antenna,transmitter and receiver.The distributed aperture deep-space radar can be equivalent to a large-scale ra-dar via coherent signal processing technology that aligning the phases of electromagnetic waves transmitted by each ra-dar.It can overcome physical limits of centralized radar system and is vividly called"China compound eye"radar be-cause its configuration is similar with compound eyes of insects.Furthermore,the recent developments of distributed ap-erture ground-based radar system are introduced.A scaled-down system composed of four 16-meter radars is completed and taken into use.Imaging experiments to the Moon have been conducted on the basis of the scaled-down system and successfully verified the feasibility of distributed aperture deep-space radar concept.Recent 2D/3D imaging results of the famous Tycho crater on the Moon are shown in this paper.Finally,the future developments of ground-based deep-space radar are considered.We believe that the distributed aperture deep-space radar system will play a critical role in planetary science and planetary defense in future.

ground-based radardeep-space detectiondistributed apertureChina Compound Eye

龙腾、丁泽刚、曾涛、董泽华、李凌豪

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北京理工大学雷达技术研究院,北京 100081

卫星导航电子信息技术教育部重点实验室(北京理工大学),北京 100081

北京理工大学重庆创新中心,重庆 401135

地基雷达 深空探测 分布孔径 中国复眼

国家自然科学基金国家自然科学基金国家自然科学基金重庆市自然科学基金

622279016210103561931002CSTB2023NSCQ-MSX0629

2024

信号处理
中国电子学会

信号处理

CSTPCD北大核心
影响因子:1.502
ISSN:1003-0530
年,卷(期):2024.40(1)
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