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A Panchromatic Imaging Fourier Transform Spectrometer for the NASA Geostationary Coastal and Air Pollution Events Mission

机译:全色成像傅里叶变换光谱仪,用于NASA对地静止的沿海和空气污染事件任务

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This paper summarizes the design and development of the Panchromatic Imaging Fourier Transform Spectrometer (PanFTS) for the NASA Geostationary Coastal and Air Pollution Events (GEO-CAPE) Mission. The PanFTS instrument will advance the understanding of the global climate and atmospheric chemistry by measuring spectrally resolved outgoing thermal and reflected solar radiation. With continuous spectral coverage from the near-ultraviolet through the thermal infrared, this instrument is designed to measure pollutants, greenhouse gases, and aerosols as called for by the U.S. National Research Council Decadal Survey; Earth Science and Applications from Space: National Imperatives for the Next Decade and Beyond1. The PanFTS instrument is a hybrid based on spectrometers like the Tropospheric Emissions Spectrometer (TES) that measures thermal emission, and those like the Orbiting Carbon Observatory (OCO), and the Ozone Monitoring Instrument (OMI) that measure scattered solar radiation. Simultaneous measurements over the broad spectral range from 1R to UV is accomplished by a two sided interferometer with separate optical trains and detectors for the UV-visible and IR spectral domains. This allows each side of the instrument to be independently optimized for its respective spectral domain. The overall interferometer design is compact because the two sides share a single high precision cryogenic optical path difference mechanism (OPDM) and metrology laser as well as a number of other instrument systems including the line-of-sight pointing mirror, the data management system, thermal control system, electrical system, and the mechanical structure. The PanFTS breadboard instrument has been tested in the laboratory and demonstrated the basic functionality for simultaneous measurements in the visible and IR. It is set to begin operations in the field at the California Laboratory for Atmospheric Remote Sensing (CLARS) observatory on Mt. Wilson measuring the atmospheric chemistry across the Los Angeles basin. Development has begun on a flight size PanFTS engineering model (EM) that addresses all critical scaling issues and demonstrates operation over the full spectral range of the flight instrument which will show the PanFTS instrument design is mature.
机译:本文概述了用于NASA对地静止沿海和空气污染事件(GEO-CAPE)任务的全色成像傅里叶变换光谱仪(PanFTS)的设计和开发。 PanFTS仪器将通过测量光谱解析出的热辐射和反射太阳辐射来增进对全球气候和大气化学的理解。该仪器具有从近紫外光到热红外的连续光谱覆盖范围,可根据美国国家研究委员会十进制调查的要求测量污染物,温室气体和气溶胶。太空中的地球科学与应用:下一个十年及以后的国家势在必行1。 PanFTS仪器是基于光谱仪(例如测量热辐射的对流层排放光谱仪(TES)以及测量散射太阳辐射的轨道碳观测站(OCO)和臭氧监测仪(OMI))的混合动力仪。通过双面干涉仪在1R到UV的宽光谱范围内同时进行测量,该干涉仪带有单独的光学系统和用于UV可见和IR光谱域的检测器。这使得仪器的每一侧都可以针对其各自的光谱域进行独立优化。整个干涉仪的设计紧凑,因为双方共享一个高精度的低温光程差机制(OPDM)和计量激光器以及许多其他仪器系统,包括视线指向镜,数据管理系统,热控制系统,电气系统和机械结构。 PanFTS面包板仪器已在实验室进行了测试,并演示了在可见光和红外光下同时进行测量的基本功能。它将开始在加利福尼亚州山顶大气遥感(CLARS)天文台的现场开展工作。威尔逊测量了整个洛杉矶盆地的大气化学。已经开始开发飞行尺寸PanFTS工程模型(EM),该模型解决了所有关键的缩放问题,并演示了飞行仪表整个光谱范围内的运行情况,这表明PanFTS仪表设计已经成熟。

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