LEO-LEO红外激光掩星大气成分探测系统设计
CSTR:
作者:
作者单位:

1中国科学院上海技术物理研究所,上海 200083;2中国科学院大学, 北京 100049;3中国科学院上海光学精密机械研究所,上海 201800;4中国科学院大气物理研究所,北京 100029;5中国科学院微小卫星创新研究院,上海 201210

作者简介:

E-mail: leiding@mail.sitp.ac.cn

通讯作者:

中图分类号:

TP394.1;TH691.9

基金项目:


Design of LEO-LEO infrared laser occultation system for atmospheric composition detection
Author:
Affiliation:

1Shanghai Institute of Technical Physics, Chinese Academy of Sciences, Shanghai 200083, China;2University of Chinese Academy of Sciences, Beijing 100049, China;3Shanghai Institute of Optics and Fine Mechanics ,Chinese Academy of Sciences, Shanghai 201800, China;4Institute of Atmospheric Physics, Chinese Academy of Sciences, Beijing 100029, China;5Innovation Academy for Microsatellite of Chinese Academy of Sciences, Shanghai 201210, China

Fund Project:

Supported by the National Key Research and Development Program of China (2024YFB3907800).

  • 摘要
  • |
  • 图/表
  • |
  • 访问统计
  • |
  • 参考文献
  • |
  • 相似文献
  • |
  • 引证文献
  • |
  • 资源附件
  • |
  • 文章评论
    摘要:

    掌握大气成分与要素在不同高度的分布特征,对于深入理解气候变化和应对气候问题具有重要作用。为了满足多大气成分(H2O、CO2、CH4、N2O、O3、CO)和视线风速垂直廓线的探测需求,开展了红外激光掩星探测系统设计。在载荷设计方面,激光发射端设计采用宽谱段频率锁定激光光源技术,制造高稳定性的红外激光;激光接收端设计采用多光栅空间外差光谱探测技术,实现较宽谱段范围、高光谱分辨率探测,光谱范围覆盖2~2.5 μm,光谱分辨率优于0.15 cm-1。在数据应用与轨道仿真方面,基于Abel变换的红外激光掩星反演方法,可实现大气成分与要素廓线在UTLS区域的同步反演;并基于仿真模拟系统进行了掩星轨道设计,经仿真分析计算掩星事件发生频次可达到61次/天,并对单次事件的数据采集过程进行了合理设计规划。

    Abstract:

    Understanding the distribution characteristics of atmospheric components and parameters at different altitudes plays a crucial role in deeply comprehending climate change and addressing climate issues. To meet the detection requirements for vertical profiles of multiple atmospheric components (H2O,CO2,CH4,N2O,O3,CO) and line-of-sight wind speed, this study designs an LEO-LEO infrared laser occultation (LIO) system. For payload design, the laser transmitter employs broadband frequency-locked laser source technology to generate highly stable infrared lasers. The receiver utilizes multi-grating spatial heterodyne spectroscopy (SHS), achieving wide spectral coverage (2-2.5 μm) and high spectral resolution (≤0.15 cm-1). For data application and orbit simulation, an Abel transform-based inversion method is proposed to synchronously retrieve atmospheric composition and parameter profiles in the Upper Troposphere and Lower Stratosphere (UTLS). Additionally, a simulated occultation orbit system demonstrates a daily occultation event frequency of up to 61 times, with optimized data acquisition processes for single events.

    参考文献
    相似文献
    引证文献
引用本文

刘云猛,黄硕,李世钊,郭慧君,余婷,王鑫,刘洋,楚晴,成龙,丁雷. LEO-LEO红外激光掩星大气成分探测系统设计[J].红外与毫米波学报,2026,45(3):528-537. Liu Yun-Meng, Huang Shuo, Li Shi-Zhao, Guo Hui-Jun, Yu Ting, Wang Xin, Liu Yang, Chu Qing, Cheng Long, Ding Lei. Design of LEO-LEO infrared laser occultation system for atmospheric composition detection[J]. J. Infrared Millim. Waves,2026,45(3):528-537.

复制
分享
相关视频

文章指标
  • 点击次数:
  • 下载次数:
  • HTML阅读次数:
  • 引用次数:
历史
  • 收稿日期:2025-05-16
  • 最后修改日期:2026-03-08
  • 录用日期:2025-07-22
  • 在线发布日期: 2026-04-03
  • 出版日期:
文章二维码