水瓶座/SAC-D微波辐射计(MWR)天线温度的初步分析:可能的天线方向图问题

S. Farrar, W. Jones
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引用次数: 4

摘要

在Aquarius/SAC-D卫星上飞行的微波辐射计(MWR)是由阿根廷航天局CONAE开发的Dicke辐射计,工作频率为23.8和36.5 GHz。该仪器补充了Aquarius (NASA的l波段辐射计/散射计),通过提供同步的空间配置环境测量,例如用于粗糙度校正的海洋风速和用于标记损坏盐度检索的降雨率。本文介绍了MWR天线波束方向图问题的初步研究结果。天线方向图的问题最好描述为不需要的地球辐射进入定向波束的侧瓣,可能是意想不到的高增益,某些MWR馈线喇叭。首先介绍一下对这个问题的理解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Preliminary analysis of the Aquarius/SAC-D Microwave Radiometer (MWR) antenna temperature: Possible antenna pattern issue
The Microwave Radiometer (MWR) flying on the Aquarius/SAC-D satellite is a Dicke radiometer operating at 23.8 and 36.5 GHz that was developed by the Argentine Space Agency CONAE. This instrument complements Aquarius (NASA's L-band radiometer/scatterometer) by providing simultaneous spatially collocated environmental measurements such as oceanic wind speed for roughness correction and rain rate for flagging corrupted salinity retrievals. This paper describes the initial findings on the MWR antenna beam pattern issue. The antenna pattern issue is best described as unwanted earth radiation entering the side-lobes of the directed beam, possibly of unexpected high gain, of certain MWR feedhorns. A first look at the understanding of this problem is presented.
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