Enabling Technologies for High Performance Microwave and MM wave Interferometric Radiometers

Hao Liu, Lijie Niu, Wei Chen, Hao Lu, Cheng Zhang, Ji Wu
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引用次数: 1

Abstract

Interferometric imaging is an alternative passive imaging method developed originally from radio astronomy from 1960’s. Comparing with the traditional real aperture system, interferometric synthetic aperture system can realize much better spatial resolution by using thinned array. Since 1980’s, this technique had been introduced in earth observation community, aiming to realize the soil moisture and ocean salinity measurement at L-band from space [1]. From 2000’s, several instrument concepts at millimeter wave (53GHz & 183GHz) had been proposed to support the next-generation geostationary orbit(GEO) meteorological satellites [2, 3, 4].
高性能微波和毫米波干涉辐射计的使能技术
干涉成像是20世纪60年代从射电天文学发展起来的一种被动成像方法。与传统的真实孔径系统相比,干涉合成孔径系统采用薄阵列,可以实现更高的空间分辨率。自20世纪80年代以来,该技术被引入对地观测界,旨在实现空间l波段土壤水分和海洋盐度的测量[1]。从2000年代开始,为了支持下一代地球静止轨道(GEO)气象卫星,已经提出了几种毫米波(53GHz和183GHz)仪器概念[2,3,4]。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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