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一种用于非局部热平衡情况下中层顶-低热层大气温度反演的新爱因斯坦系数方法。

A new Einstein coefficient method for mesopause-lower thermosphere atmosphere temperature retrieval under a non-local thermal equilibrium situation.

作者信息

Li Haotian, Feng Yutao, Li FaQuan, Wang Houmao, Hu Xiangrui, He Weiwei, Wu Kuijun

出版信息

Opt Express. 2023 Sep 11;31(19):30413-30434. doi: 10.1364/OE.498765.

DOI:10.1364/OE.498765
PMID:37710583
Abstract

The mesopause-lower thermosphere (MLT) region is an important spatial region in the Earth's atmosphere, making it a valuable area to investigate the temperature variations. Kirchhoff's law fails with the altitude increase due to the non-local thermal equilibrium effect, resulting in an increase in the error of the method to retrieve the atmospheric temperature in the MLT region using the A-band spectral line intensity. In the non-LTE state, the temperature retrieval method based on the Einstein coefficients is proposed to retrieve atmospheric temperature in the 92-140 km height range using the airglow radiation intensity images obtained from the Michelson Interferometer for global high-resolution thermospheric imaging (MIGHTI) measurements. Results show that the temperature deviation of the two-channel combinations does not exceed 15 K in the altitude range of 92-120 km. This deviation increases up to 45 K when the altitude is in the range of 120-140 km due to the influence of the N airglow spectrum. The two-channel combinations self-consistency is increased by 85 K compared with the temperature obtained using the spectral line intensity retrieval. Additionally, the comparison of the retrieval results with the spectral line intensity method and the comparison with the atmospheric chemistry experiment Fourier transform spectrometer (ACE-FTS) temperature measurement data shows that the Einstein coefficient method is significantly more rational and accurate than the spectral line intensity method.

摘要

中间层顶-低热层(MLT)区域是地球大气中的一个重要空间区域,使其成为研究温度变化的重要区域。由于非局部热平衡效应,基尔霍夫定律随着海拔升高而失效,导致利用A波段谱线强度反演MLT区域大气温度的方法误差增大。在非局部热平衡(non-LTE)状态下,提出了基于爱因斯坦系数的温度反演方法,利用从用于全球高分辨率热层成像的迈克尔逊干涉仪(MIGHTI)测量中获得的气辉辐射强度图像,反演92-140千米高度范围内的大气温度。结果表明,在92-120千米高度范围内,双通道组合的温度偏差不超过15K。由于N气辉光谱的影响,当海拔在120-140千米范围内时,该偏差增大到45K。与利用谱线强度反演得到的温度相比,双通道组合的自洽性提高了85K。此外,将反演结果与谱线强度法进行比较,并与大气化学实验傅里叶变换光谱仪(ACE-FTS)温度测量数据进行比较,结果表明爱因斯坦系数法比谱线强度法明显更合理、更准确。

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