首页|痕量气体掩星探测高光谱成像光谱仪光学系统设计

痕量气体掩星探测高光谱成像光谱仪光学系统设计

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痕量气体作为大气的重要成份,对地球的生态起着重要作用.为了实现宽波段、高光谱全天时连续测量,本文设计了一款在掩星探测模式下工作的高光谱成像光谱仪.该系统为共狭缝的双通道结构,紫外-可见光通道采用单凹面光栅结构、红外通道采用利特罗与浸没光栅结合结构,有效地减小了体积.利用软件对光学结构进行优化,优化结果表明:光谱仪在 250~952 nm波段范围内工作,其中紫外-可见光通道工作波段为 250~675 nm、光谱分辨率优于 1 nm、MTF在奈奎斯特频率为 20 lp/mm处均高于 0.58、全视场各波长处RMS值均小于 21 μm;红外通道工作波段为 756~952 nm、光谱分辨率优于 0.2 nm、MTF在奈奎斯特频率为 20 lp/mm处均高于 0.76、全视场各波长处RMS值均小于 6 μm,均满足设计要求.结果表明该高光谱成像光谱仪系统可以实现对痕量气体的掩星探测.
Optical system design of hyperspectral imaging spectrometer for trace gas occultation detection
Trace gases,as important constituents of the atmosphere,play an important role in the ecology of the planet.In order to realize the requirements of wide-band,hyperspectral and all-weather continuous meas-urement,a hyperspectral imaging spectrometer operating in occultation detection mode is designed in this pa-per.The system is a dual-channel structure with a common slit,the UV-visible channel adopts a single con-cave grating,and the infrared channel adopts a structure combining Littrow and immersion grating,which ef-fectively reduces the volume.The software is used to optimize the optical structure,and the optimization res-ults show that the spectrometer operates in the range of 250-952 nm wavelengths,of which the UV-visible channel operates in the wavelength range of 250-675 nm,the spectral resolution is better than 1 nm,the MT-Fs are all higher than 0.58 at a Nyquist frequency of 20 lp/mm,and the RMS values at various wavelengths of the full-field-of-view are all less than 21 μm;the infrared channel operates in the wavelength band of 756-952 nm,the spectral resolution is better than 0.2 nm,the MTF is higher than 0.76 at the Nyquist fre-quency of 20 lp/mm,and the RMS value at each wavelength in the whole field of view is less than 6 μm,all of them meet the design requirements.It can be seen that the hyperspectral imaging spectrometer system can realize the occultation detection of trace gases.

optical system designoccultation detectiontrace gashyperspectral imaging spectrometer

孔相金、李博、李寒霜、王晓旭、顾国超、蒋雪

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中国科学院长春光学精密机械与物理研究所,吉林长春 130033

中国科学院大学,北京 100049

光学系统设计 掩星探测 痕量气体 高光谱成像光谱仪

国家重点研发计划国家自然科学基金

2022YFB390320262205330

2024

中国光学
中国科学院长春光学 精密机械与物理研究所 中国光学学会

中国光学

CSTPCD北大核心
影响因子:2.02
ISSN:2095-1531
年,卷(期):2024.17(3)
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