Geophysical Model Functions of Ocean Surface Winds for the Meteor-M No. 2 MTVZA-GY Radiometer

L. Mitnik, V. Kuleshov, M. Mitnik, M. Pichugin, G. M. Chernyavsky, I. V. Cherny, O.V. Nikitin
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Abstract

The MTVZA-GY microwave radiometer on board the Russian Meteor-M No. 2 meteorological space apparatus is the single instrument scanning the Earth under the incidence angle of 65°. The geophysical model function (GMF) relating the MTVZA-GY brightness temperatures TB(v) to the sea surface wind speed at the frequencies v between 10 and 36 GHz was derived by the joint analysis of the TB(v), the scatterometer and ERA5 reanalysis data. The reanalysis data were used to found the total cloud absorption and atmospheric contributions to the measured TB(s) and compute the brightness temperature of the ocean surface under various wind speeds. The collocated database included also the GCOM-W1 AMSR2 TB(v) and was obtained for winter deep cyclones in the Northern Pacific Ocean.
气象- m 2号MTVZA-GY辐射计海洋表面风的地球物理模式函数
俄罗斯气象- m 2号气象空间仪器上的MTVZA-GY微波辐射计是在65°入射角下对地球进行扫描的单一仪器。通过对TB(v)、散射计和ERA5再分析资料的联合分析,导出了10 ~ 36 GHz频率v范围内MTVZA-GY亮温TB(v)与海面风速的地球物理模型函数(GMF)。利用再分析数据计算了总云吸收和大气对测量TB(s)的贡献,并计算了不同风速下海洋表面的亮温。该数据库还包括GCOM-W1 AMSR2 TB(v),该数据库是为北太平洋冬季深层气旋而获得的。
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