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

机译:深度空间校准运动过程中TRMM微波成像仪天线温度的估计

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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,热带降雨测量特派团观测台已经表演了一组称为深空间校准(DSC)的一组机动,允许TRMM微波成像仪圆锥扫描天线梁查看2.7 kelvin的已知的非极化校准场景。然而,在此期间,辐射传递函数(辐射计数到Ta)仅对主要反射器深空视图的非常短的部分仅适用于。本文讨论了重建辐射传递函数的三种方法,从而为绝对校准提供更长的天线温度(TA)的时间序列。在本文中确认了进入天线图案的饲料溢出区域的地球发射。这项工作的动机是制定2014年5月设定的全球降水测量(GPM)微波成像器(GMI)DSC机动。

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