Low SWaP hyperspectral imaging sensor for CubeSat applications

I. Bendoym, Lori A. Lepak, J. Leitch, J. Applegate, D. Crouse
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Abstract

The health of Earth’s atmosphere and its ecosystems are of vital importance to humanity. To assess the current state of the atmosphere and its rate of degradation, the monitoring of atmospheric gasses and particulates is necessary. The development of next-generation Low size, weight, and power (SWaP) sensors and instruments which are required for this task is a high priority for NASA’s Earth Science Technology Office (ESTO). The primary tool to monitor atmospheric gasses is hyperspectral imaging (HSI). Current HSI systems are composed of a large and complex assortment of lenses, filters and cameras that are large, heavy, expensive, and intolerant to physical shocks—all things that make them challenging for use in space-based sensing and imaging applications. As an alternative, a Low SWaP sensor is made possible by integrating a compact HSI sensor onto a CubeSat or SmallSat platform, which is much cheaper to deploy vs. a conventional satellite. To facilitate this, metamaterials are employed at the detector level to reduce the optical components required for HSI, while still providing comparable performance. The metamaterial studied here replaces a conventional grating disperser in a HSI system, by being compatible with a focused beam (fast optics) while spectrally filtering a particular spectral channel.
用于立方体卫星应用的低SWaP高光谱成像传感器
地球大气及其生态系统的健康对人类至关重要。为了评估大气的现状及其退化速度,必须对大气气体和微粒进行监测。该任务所需的下一代低尺寸、低重量、低功耗(SWaP)传感器和仪器的开发是NASA地球科学技术办公室(ESTO)的重中之重。监测大气气体的主要工具是高光谱成像(HSI)。目前的HSI系统由大量复杂的镜头、滤镜和相机组成,这些镜头、滤镜和相机体积大、重量重、价格昂贵,而且不能承受物理冲击——所有这些都使它们在天基传感和成像应用中具有挑战性。作为替代方案,通过将紧凑型HSI传感器集成到CubeSat或SmallSat平台上,可以实现低SWaP传感器,与传统卫星相比,这种传感器的部署成本要低得多。为了实现这一点,在探测器级使用超材料来减少HSI所需的光学元件,同时仍然提供相当的性能。本文研究的超材料通过与聚焦光束(快速光学)兼容,同时对特定的光谱通道进行光谱滤波,取代了HSI系统中的传统光栅分散器。
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