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EuRAD01 : EuRAD Opening Session

机译:欧元欧元:欧元开幕式会议

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Radar instruments play a critical role in NASA's planetary, cometary, and Earth observing missions. Sometimes they guide space crafts to the surface of another planet (such as Mars) or a comet and some other times they are used for answering fundamental scientific questions by exploring cometary and planetary bodies, including our own Earth. Until recently, the majority of NASA's radar instruments were below 100 GHz. However, in recent years, there has been a lot of interest in using millimeter-wave and terahertz radars to answer critical scientific questions. One such instrument developed by us is a 183 GHz (G-Band) differential absorption radar providing a new measurement capability of simultaneously measuring water vapor and ice content in clouds in Earth's atmosphere with high precision and spatial resolution. Profiling of water vapor within clouds is a critical requirement to address the key unsolved science questions regarding the processes regulating cloud lifecycle and the transport of water vapor by convection. Another instrument we developed is a 90 GHz (W-Band) frequency modulated continuous wave (FMCW) radar for understanding the origin, dynamics, and evolution of jets from a comet. When deployed, this will provide clues to the formation of comets and therefore the early stages of the Solar System. The same W-band radar is also being planned for investigating plumes on icy moons, such as Europa and Enceladus, which will shed light on subsurface processes and structure on these potentially life-harboring bodies. We are also building a revolutionary in situ radar instrument for short-range mapping of near-surface atmospheric water vapor on Mars. This highly compact and low-power differential absorption radar operates near the 557 GHz water absorption line to measure absolute humidity along its beam path with as good as few-ppm level accuracy. This instrument allows us, for the first time, range-resolved absolute humidity estimates on Martian surface. Apart from science instrument radars, we also developed a 670 GHz FMCW radar for imaging at stand-off distances for security applications.
机译:雷达仪器在美国宇航局的行星,彗星和地球观察任务中发挥着关键作用。有时,他们将空间工艺引导到另一个星球的表面(如火星)或彗星,一些其他时间通过探索包括我们自己的地球的彗星和行星机构来回答基本科学问题。直到最近,大多数美国宇航局的雷达仪器低于100 GHz。然而,近年来,使用毫米波和太赫兹雷达已经有很多兴趣回答关键的科学问题。由我们开发的一种这样的仪器是183 GHz(G波段)差动吸收雷达,提供了具有高精度和空间分辨率的地球大气中云中的水蒸气和冰含量的新测量能力。云内的水蒸气分析是解决关于调节云生命周期的过程和通过对流运输水蒸气的关键未解决的科学问题的重要要求。我们开发的另一种仪器是90 GHz(W波段)频率调制的连续波(FMCW)雷达,用于了解彗星的起源,动力学和喷射器的演化。部署时,这将为彗星形成的线索提供线索,从而为太阳系的早期阶段提供。相同的W波段雷达也计划用于调查冰冷的卫星上的羽毛,例如Europa和Enceladus,这将在这些潜在的寿命尸体上阐明地下过程和结构。我们还在建立一个革命性的火星近表面大气水蒸气的短程雷达仪器。这种高度紧凑且低功耗的差动吸收雷达在557GHz吸水管线附近运行,以沿着其光束路径测量绝对湿度,与少数PPM的水平精度一样好。该仪器允许我们第一次进行Ranget-Sollat​​ive的绝对湿度估计。除了科学仪器雷达之外,我们还开发了一个670 GHz FMCW雷达,用于在脱扣距离处进行成像,用于安全应用。

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    《European Radar Conference》|2021年|1-139|共139页
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