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首页> 外文期刊>Remote Sensing >Concept Development and Risk Reduction for MISTiC Winds, A Micro-Satellite Constellation Approach for Vertically Resolved Wind and IR Sounding Observations in the Troposphere
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Concept Development and Risk Reduction for MISTiC Winds, A Micro-Satellite Constellation Approach for Vertically Resolved Wind and IR Sounding Observations in the Troposphere

机译:MISTiC风的概念发展和风险降低,一种对流层垂直分辨风和红外测深观测的微卫星星座方法

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摘要

MISTiC Winds is an instrument and constellation mission approach to simultaneously observe the global thermodynamic state and the vertically resolved horizontal wind field in the troposphere from LEO SSO. The instrument is a wide-field imaging spectrometer operated in the 4.05–5.75 μm range, with the spectral resolution, sampling, radiometric sensitivity, and stability needed to provide temperature and water vapor soundings of the atmosphere, with 1 km vertical resolution in the troposphere-comparable to those of NASA’s atmospheric infrared sounder (AIRS). These instruments have much higher spatial resolution (3 km at nadir) and finer spatial sampling than current hyperspectral sounders, allowing a sequence of such observations from several micro-satellites in an orbital plane with short time separation, from which atmospheric motion vector (AMV) winds are derived. AMVs for both cloud-motion and water vapor-motion, derived from hyperspectral imagery, will have improved velocity resolution relative to AMVs obtained from multi-spectral instruments operating in GEO. MISTiC’s extraordinarily small size, low mass (15 kg), and minimal cooling requirements can be accommodated aboard an ESPA-class microsatellite. Low fabrication and launch costs enable this constellation to provide more frequent atmospheric observations than current-generation sounders provide, at much lower mission cost. Key technology and observation method risks have been reduced through recent laboratory and airborne (NASA ER2) testing funded under NASA’s Instrument Incubator Program and BAE Systems IR&D, and through an observing system simulation experiment performed by NASA GMAO. This approach would provide a valuable new capability for the study of the processes driving high-impact weather events, and critical high-resolution observations needed for future numerical weather prediction.
机译:MISTiC Winds是一种仪器和星座任务方法,可同时从LEO SSO观测对流层的整体热力学状态和垂直解析的水平风场。该仪器是在4.05–5.75μm范围内运行的宽视场成像光谱仪,具有提供大气温度和水汽探测所需的光谱分辨率,采样,辐射敏感性和稳定性,对流层的垂直分辨率为1 km -与NASA的大气红外测深仪(AIRS)相比。与目前的高光谱测深仪相比,这些仪器具有更高的空间分辨率(天底<3 km)和更精细的空间采样,从而可以在较短的时间间隔内从轨道平面中的几个微卫星进行一系列这样的观测,从而与大气运动矢量(AMV) )产生了风。相对于从在GEO中运行的多光谱仪器获得的AMV,来自高光谱影像的用于云运动和水蒸气运动的AMV的速度分辨率将得到改善。 MISTiC的体积特别小,重量轻(<15千克),并且冷却要求最低,可以在ESPA级微型卫星上使用。较低的制造和发射成本使该星座能够以比目前的探空仪更高的任务成本提供更频繁的大气观测。通过最近由NASA仪器孵化器计划和BAE Systems IR&D资助的实验室和机载(NASA ER2)测试,以及通过NASA GMAO进行的观测系统模拟实验,降低了关键技术和观测方法的风险。这种方法将为研究驱动高影响天气事件的过程以及未来数值天气预报所需的关键高分辨率观测提供新的有价值的功能。

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