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Assessment and Adaptive Correction of Observations in Atmospheric Sounding Channels of the Satellite Microwave Radiometer MTVZA-GY

机译:卫星微波辐射计大气探测渠道的评估与自适应校正MTVZA-GY

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摘要

The microwave radiometer MTVZA-GY on board the Russian polar orbiting meteorological satellite Meteor-M N2 is briefly described. Errors and biases in antenna brightness temperatures are documented. Observation errors are found to be dependent on the solar angles. An adaptive bias correction technique for MTVZA-GY antenna temperatures is motivated and developed. The technique accounts for the solar angles and sequentially assimilates observed minus simulated radiances in a perpetual 24 h cycle in order to estimate up-to-date correction coefficients defined to be functions of the zenith and azimuth solar angles. The simulated radiances are computed by the RTTOV radiative transfer model from three-dimensional numerical weather prediction fields. The correction technique is implemented for atmospheric temperature and humidity sounding channels of MTVZA-GY. The corrected observations are shown to be significantly more accurate as compared with raw antenna temperatures and with observations that undergo simpler and more traditional corrections. The accuracy of corrected MTVZA-GY observations is compared with the accuracy of AMSU-A and MHS data.
机译:简要描述了俄罗斯极地轨道气象卫星Meteor-M N2上的微波辐射计MTVZA-GY。记录了天线亮度温度的错误和偏差。发现观察误差取决于太阳角。用于MTVZA-GY天线温度的自适应偏压校正技术是动力和开发的。该技术考虑了太阳角度并依次同化观察到的减去长期24小时循环中的模拟辐射,以便估计定义为Zenith和方位角太阳角的功能的最新校正系数。模拟的辐射由来自三维数值天气预报领域的RTTOV辐射传输模型计算。校正技术用于MTVZA-GY的大气温度和湿度探测通道。与原始天线温度相比,校正的观察结果明显更准确,并且观察到经历更简单和更传统的校正。将校正MTVZA-GY观察的准确性与AMSU-A和MHS数据的准确性进行比较。

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