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THE INFRARED ATMOSPHERIC SOUNDER ONBOARD FY-3A SATELLITE

机译:红外大气探测器FY-3A卫星

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FY-3Am eteorological satellite is the second generation of polar -orbit meteorological satellite in China which plans to be launched in May , 2008. It loads 11 instruments and some new instrum ents are carried for the first time. IRAS is one of the atmospheric vertical sounding instrum ents, its aim is providing multi-channel brightness temperature that in the spectra 1 ra nge of visi ble to long -wave infrared for direct radiance assimilation and retrievals of global arm ospheric temperature profiles, humidity profiles, ozone column contents, cloud param eters ,etc. The spectr al channels and instru ment configuration of IRAS are designed sim ilar to HIRS instrum ent that onboard NOAA polar-orbit satellite series. This paper give a introduction about IRAS de signed instrument configuration, and some pre-launch study results about system spectral response function, laboratory infrared radiometric calibration, laboratory visible and near infrared integrating sphere calibration.
机译:FY-3Am气象卫星是中国第二代极轨气象卫星,计划于2008年5月发射。它装载11台仪器,并且首次携带一些新仪器。 IRAS是大气垂直探测仪器之一,其目的是提供可见光到长波红外光谱范围内的多通道亮度温度,以直接吸收辐射并获取全球手臂大气温度分布图,湿度分布图。 ,臭氧柱含量,云参数等IRAS的光谱通道和仪器配置的设计类似于HIRS仪器,它与NOAA极轨道卫星系列相同。本文介绍了IRAS设计的仪器配置,以及有关系统光谱响应函数,实验室红外辐射定标,实验室可见光和近红外积分球定标的一些启动前研究结果。

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