综述与评述

红外高光谱被动遥感气溶胶研究现状及进展

  • 胡帅 ,
  • 赵嘉琦 ,
  • 刘磊 ,
  • 党蕊君 ,
  • 肖瑶 ,
  • 何钰龙
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  • 1.国防科技大学 气象海洋学院,湖南 长沙 410073
    2.中国气象局高影响天气(专项) 重点开放实验室,湖南 长沙 410073
胡帅,主要从事大气辐射与遥感研究. E-mail: hushuai2012@nudt.edu.cn
赵嘉琦,主要从事大气辐射与遥感研究. E-mail: zhaojiaqi17@nudt.edu.cn

收稿日期: 2025-08-27

  修回日期: 2025-10-21

  网络出版日期: 2025-11-01

基金资助

国家自然科学基金项目(42175154);湖南省杰出青年基金项目(2024JJ2058)

Current Status and Progress of the Infrared Hyperspectral Passive Remote Sensing of Atmospheric Aerosol

  • Shuai HU ,
  • Jiaqi ZHAO ,
  • Lei LIU ,
  • Ruijun DANG ,
  • Yao XIAO ,
  • Yulong HE
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  • 1.School of Meteorology and Oceanography, National University of Defense Technology, Changsha 410073, China
    2.Key Laboratory of High Impact Weather (special), China Meteorological Administration, Changsha 410073, China
HU Shuai, research areas include atmospheric radiation and remote sensing. E-mail: hushuai2012@nudt.edu.cn
ZHAO Jiaqi, rsearch areas include atmospheric radiation and remote sensing. E-mail: zhaojiaqi17@nudt.edu.cn

Received date: 2025-08-27

  Revised date: 2025-10-21

  Online published: 2025-11-01

Supported by

the National Natural Science Foundation of China(42175154);The Science Foundation of Hunan Province(2024JJ2058)

摘要

气溶胶是影响地气系统能量收支及大气环境变化的关键因子之一,其光学参数的高精度反演一直是大气环境遥感领域的研究热点之一。气溶胶光学被动遥感主要利用其在可见光/近红外波段的散射效应,但该方式大多需要借助太阳散射辐射作为辐射源,在夜间和高纬度冬季(极夜)无法适用。红外高光谱遥感技术可解析气溶胶独特的光谱吸收与散射指纹特征,也是实现气溶胶遥感的手段之一,为传统可见光/近红外反演遥感提供了有力补充。系统阐述了红外高光谱反演气溶胶微物理参数的基本原理,重点对物理机理与探测仪器、辐射传输模型和反演算法等方面的关键技术进行综述。尤其是对已有红外高光谱辐射计的关键参数、红外高光谱正向辐射传输模型的特点以及不同类型反演方法的优缺点进行了探讨分析。基于此,进一步展望了未来研究的发展方向,提出应重点发展高精度、高效率的辐射传输正演模型,深度挖掘红外高光谱数据中的丰富信息以改进反演算法,并积极发展多平台协同探测技术。

本文引用格式

胡帅 , 赵嘉琦 , 刘磊 , 党蕊君 , 肖瑶 , 何钰龙 . 红外高光谱被动遥感气溶胶研究现状及进展[J]. 地球科学进展, 2025 , 40(11) : 1097 -1111 . DOI: 10.11867/j.issn.1001-8166.2025.098

Abstract

Aerosols are key factors influencing the energy balance of the Earth-atmosphere system and atmospheric environmental changes. High-precision inversion of their optical parameters has long been a topic of interest in atmospheric environmental remote sensing. Passive remote sensing of aerosol optics primarily utilizes their scattering effects in the visible/near-infrared wavelength bands. However, this approach typically relies on solar scattered radiation as the radiation source, rendering it inapplicable at night and during high-latitude winters (polar nights). Infrared hyperspectral remote sensing technology can resolve the unique spectral absorption and scattering fingerprint characteristics of aerosols, serving as another means to achieve aerosol remote sensing and providing a powerful supplement to traditional visible/near-infrared inversion techniques. This paper systematically elaborates on the fundamental principles of infrared hyperspectral inversion for aerosol microphysical parameters, focusing on key technologies such as physical mechanisms and detection instruments, radiative transfer models, and inversion algorithms. Particular emphasis is placed on discussing the key parameters of existing hyperspectral radiometers, the characteristics of hyperspectral forward radiative transfer models, and the advantages and disadvantages of different inversion methods. Based on this, the paper further outlines future research directions, proposing a focus on developing high-precision, high-efficiency forward radiative transfer models, utilizing the rich information within hyperspectral data to improve inversion algorithms, and actively advancing multi-platform collaborative detection technologies.

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