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Estimation of TRMM microwave imager antenna temperature during Deep Space Calibration maneuvers

机译:太空校准演习中TRMM微波成像仪天线温度的估算

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In 1998, the Tropical Rainfall Measuring Mission observatory performed a set of maneuvers known as Deep Space Calibration (DSC) that allowed the TRMM Microwave Imager conically scanning antenna beam to view a known non-polarized calibration scene of 2.7 Kelvin. However, during this period the radiometric transfer function (radiometric counts-to-TA) was only valid for only a very short portion of main reflector deep space view. This paper discusses three methods of reconstructing the radiometric transfer function thereby providing a longer time series of Antenna Temperature (TA) for absolute calibration. Earth emission entering into the feed spillover region of the antenna pattern is acknowledged within this paper. The motivation of this work is for preparation of the Global Precipitation Measurement (GPM) Microwave Imager (GMI) DSC maneuvers set for May of 2014.
机译:1998年,热带降雨测量团天文台执行了一系列称为深空校准(DSC)的操作,该操作使TRMM微波成像仪以圆锥形方式扫描天线波束,以查看已知的2.7开尔文的非偏振校准场景。但是,在此期间,辐射传递函数(对TA的辐射计数)仅对主反射器深空视图的一小部分有效。本文讨论了三种重建辐射传递函数的方法,从而为绝对校准提供了更长的天线温度(TA)时间序列。本文确认了进入天线方向图的馈电溢出区域的地球发射。这项工作的目的是为定于2014年5月进行的全球降水测量(GPM)微波成像仪(GMI)DSC演习做准备。

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