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PAU-SA: A Synthetic Aperture Interferometric Radiometer Test Bed for Potential Improvements in Future Missions

机译:PAU-SA:用于未来任务的潜在改进的合成孔径干涉辐射计测试台

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摘要

The Soil Moisture and Ocean Salinity (SMOS) mission is an Earth Explorer Opportunity mission from the European Space Agency (ESA). Its goal is to produce global maps of soil moisture and ocean salinity using the Microwave Imaging Radiometer by Aperture Synthesis (MIRAS). The purpose of the Passive Advanced Unit Synthetic Aperture (PAU-SA) instrument is to study and test some potential improvements that could eventually be implemented in future missions using interferometric radiometers such as the Geoestacionary Atmosferic Sounder (GAS), the Precipitation and All-weather Temperature and Humidity (PATH) and the Geostationary Interferometric Microwave Sounder (GIMS). Both MIRAS and PAU-SA are Y-shaped arrays with uniformly distributed antennas, but the receiver topology and the processing unit are quite different. The purpose of this work is to identify the elements in the MIRAS's design susceptible of improvement and apply them in the PAU-SA instrument demonstrator, to test them in view of these future interferometric radiometer missions.
机译:土壤水分和海洋盐度(SMOS)任务是欧洲航天局(ESA)的“地球探索者机会”任务。其目标是使用光圈合成(MIRAS)的微波成像辐射计绘制全球土壤湿度和海洋盐度地图。被动式先进单位合成孔径(PAU-SA)仪器的目的是研究和测试一些潜在的改进,这些改进最终可能会在未来的任务中使用干涉辐射计(例如地球静止大气震荡仪(GAS),降水和全天候测量仪)实施温湿度(PATH)和地球静止干涉微波测深仪(GIMS)。 MIRAS和PAU-SA都是Y形阵列,天线分布均匀,但是接收器拓扑和处理单元却大不相同。这项工作的目的是确定MIRAS设计中有待改进的元素,并将其应用到PAU-SA仪器演示器中,以便根据未来的干涉式辐射计任务进行测试。

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