大气红外探空仪(AIRS)多孔径光谱仪设计

R. Pagano, M. Hatch
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引用次数: 3

摘要

准确了解地球垂直大气温度结构是数值天气预报的基础。美国国家气象局(NWS)提出了在整个对流层实现1度精度和1公里垂直分辨率的温度探测的最终目标。为了实现这一目标,下一代温度测深仪必须增加光谱覆盖范围和光谱分辨率。大量仿真结果表明,光谱分辨能力(λ/Δλ)为1200,波长覆盖范围为3.4 ~ 17 μm的温度测深仪可显著提高rms温度反演精度。用于地球观测系统(Eos)的大气红外探测器(AIRS)就是为了满足这些需求而设计的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Multi-Aperture Spectrometer Design for the Atmospheric Infrared Sounder (AIRS)
Accurate knowledge of the Earth's vertical atmospheric temperature structure is fundamental to numerical weather prediction. The National Weather Services (NWS) have stated an ultimate goal for temperature sounding of 1 degree accuracy and 1 km vertical resolution throughout the troposphere. To approach this goal next generation temperature sounders must have increased spectral coverage and increased spectral resolution. Extensive simulations indicate that a temperature sounder with spectral resolving power (λ/Δλ) of 1200 and wavelength coverage from 3.4 - 17 μm will significantly improve the rms temperature retrieval accuracy. The Atmospheric Infrared Sounder (AIRS) for the Earth Observing System (Eos) has been designed to meet these requirements.
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