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Optical design of the composite infrared spectrometer (CIRS) for the Cassini mission

机译:Cassini Mission的复合红外光谱仪(CIRS)的光学设计

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The Composite Infrared Spectrometer (CIRS) is an instrument currently under development at NASA Goddard Space Flight Center for the Cassini mission to Saturn. The CIRS optical design heritage extends back to the Infrared Interferometer Spectrometer (IRIS) which flew on Voyager. CIRS is the next logical step in the exploration of the atmosphere of Saturn and Titan. It will obtain more complete sets of data with broader spectral coverage, higher spectral and spatial resolution, and greater sensitivity. The CIRS optical design consists of four subassemblies: (1) a 50.8 cm diameter Cassegrain telescope, (2) a Mid-Infrared (MIR) Michelson interferometer, (3) a Far-Infrared (FIR) polarizing interferometer, and (4) a Reference interferometer (RI).
机译:复合红外光谱仪(CIRS)是目前在NASA戈达德太空飞行中心开发的仪器,为Cassini Mission到土星。 CIRS光学设计遗传延伸回红外干涉仪光谱仪(IRIS),飞行于航行员。 Cirs是探索土星和泰坦氛围中的下一个逻辑步骤。它将获得更完整的数据集,具有更广泛的光谱覆盖,更高的光谱和空间分辨率,更高的灵敏度。 CIRS光学设计由四个子组件组成:(1)直径50.8厘米直径的Cassegrain望远镜,(2)中红外(MIR)Michelson干涉仪,(3)远红外(FIR)偏振干涉仪,(4)a参考干涉仪(RI)。

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