温室气体监测仪器的在轨光谱特性分析:光谱波长稳定性和仪器线形稳定性

IF 2.2 3区 物理与天体物理 Q2 OPTICS
Yunfei Han , Hailiang Shi , Zhiwei Li , Haiyan Luo , Xianhua Wang , Hanhan Ye , Yi Ding , Feng Zhu , Shichao Wu , Wei Xiong
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引用次数: 0

摘要

温室气体监测仪器(GMI)是根据空间外差分光技术原理开发的碳卫星有效载荷,专门用于全球温室气体(二氧化碳和甲烷)"源 "和 "汇 "的分析。由于二氧化碳和甲烷在大气中的浓度较低且梯度变化极小,因此需要更高的精度来对其进行检索。卫星发射过程中的振动和在轨运行期间恶劣的空间环境可能会导致各种有效载荷组件的性能发生变化,从而降低光谱产品的质量和回收精度。本文提出了一套为全球监测仪量身定制的在轨光谱特性评估方法,以监测其光谱质量。本文还专门为全球海洋监测仪开发了一种自适应盲像素检测和校正算法,并优化了干涉图处理流程算法。进行了在轨光谱校准,并建立了评估光谱特征参数的方法。分析的重点是全球海洋监测仪 CO2-1 波段(1.575 μm)的光谱特性在一年在轨校准光谱期间的变化。进入轨道后的初始光谱波长偏移为 0.133 厘米-1,稳定运行期间的平均光谱波长偏移为 0.0313 厘米-1。在一年的时间里,全球监测仪仪器线形函数的最大变化为 0.006 厘米-1。在天底观测模式下获得的观测光谱经过了精度验证。结果表明,光谱峰值波数以及观测光谱和理论光谱的相对趋势变化是一致的,平均相对残差为 0.987%。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
On-orbit spectral characteristics analysis of the greenhouse gases monitoring instrument: Spectral wavelength stability and instrumental line shape stability
The Greenhouse Gases Monitoring Instrument (GMI) is a carbon satellite payload developed based on the principle of spatial heterodyne spectroscopy technology, which is specifically designed for the global analysis of greenhouse gases (CO2 and CH4) “sources” and “sinks”. Due to the low concentration and minimal gradient variations of CO2 and CH4 in the atmosphere, higher precision is required for their retrieval. Vibrations during satellite launch and harsh space environments during on-orbit operation may cause changes in the performance of various payload components, resulting in decreased quality of spectrum products and retrieval precision. This paper proposes a set of on-orbit spectral characteristic evaluation methods tailored for the GMI to monitor the quality of its spectrum. It also develops an adaptive blind pixel detection and correction algorithm specifically for the GMI and optimizes the interferogram processing flow algorithm. On-orbit spectral calibration is performed, and methods to evaluate spectral characteristic parameters have been established. The analysis focuses on the variations of the spectral characteristics in the CO2-1 bands (1.575 μm) of the GMI during one-year of on-orbit calibration spectrum. The initial spectral wavenumber offset is 0.133 cm−1 after entering orbit, and the average spectral wavenumber offset is 0.0313 cm−1 during stable operation. During the one-year period, the maximum variation in the instrumental line shape function of the GMI is 0.006 cm−1. The observed spectrum obtained in nadir observation mode, underwent to accuracy verification. The results demonstrate consistency between the spectral peak wavenumbers and the relative trend changes of the observed and theoretical spectrum, with an average relative residual of 0.987%.
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来源期刊
Optics Communications
Optics Communications 物理-光学
CiteScore
5.10
自引率
8.30%
发文量
681
审稿时长
38 days
期刊介绍: Optics Communications invites original and timely contributions containing new results in various fields of optics and photonics. The journal considers theoretical and experimental research in areas ranging from the fundamental properties of light to technological applications. Topics covered include classical and quantum optics, optical physics and light-matter interactions, lasers, imaging, guided-wave optics and optical information processing. Manuscripts should offer clear evidence of novelty and significance. Papers concentrating on mathematical and computational issues, with limited connection to optics, are not suitable for publication in the Journal. Similarly, small technical advances, or papers concerned only with engineering applications or issues of materials science fall outside the journal scope.
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