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Optical assembly of a visible-through-thermal infrared multispectral imaging system

机译:可见光-热红外多光谱成像系统的光学组件

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Abstract: The Optical Assembly (OA) for the Multispectral Thermal Imger (MTI) program has been fabricated, assembled, and successfully tested for its performance. It represents a major milestone achieved towards completion of this earth observing EO imaging sensor that is to be operated in low earth orbit. Along with its wide field of view, 1.82 degrees along-track and 1.38 degrees cross-track, and comprehensive on-board calibration system, the pushbroom imaging sensor employs a single mechanically cooled focal plane with 15 spectral bands covering a wavelength range from 0.45 to 10.7 $mu@m. The OA has an off-axis three-mirror anastigmatic telescope with a 36-cm unobscured clear aperture. The two key performance criteria, 80 percent enpixeled energy in the visible and radiometric stability of 1 percent 1 $sigma in the visibleear-IR and short wavelength IR, of 1.45 percent 1 $sigma in the medium wavelength IR, and of 0.53 percent 1 $sigma long wavelength IR, as well as its low weight and volume constraint drive the overall design configuration of the OA and fabrication requirements. !4
机译:摘要:已经制造,组装并成功测试了多光谱热Imger(MTI)程序的光学组件(OA)。这是该地球观测EO成像传感器完成的主要里程碑,该传感器将在低地球轨道上运行。凭借其广阔的视野,1.82度的横向航迹和1.38度的横向航迹以及全面的车载校准系统,推扫成像传感器采用了一个机械冷却的焦平面,该焦平面具有15个光谱带,涵盖了从0.45到0.55的波长范围。 10.7美元/平方米。 OA具有离轴三镜无像镜望远镜,该望远镜具有36厘米的透明光圈。这两个关键性能标准是可见光和辐射稳定度中80%的像素能量,可见光/近红外和短波长IR中为1%1 sigma,中波长IR中为1.45%1 sigma,0.53% 1 $ sigma长波长IR以及其低的重量和体积限制驱动了OA的总体设计配置和制造要求。 !4

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