Inversion of O_(2) 1.27 μm nightglow emissions: A climatological analysis using satellite Limb-Viewed spectra and Harmonic analysis method  

作　　者：YiYi Sui YaJun Zhu QiuYu Chen MaoSheng He JiYao Xu 

机构地区：[1]State Key Laboratory of Space Weather,National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China [2]University of Chinese Academy of Sciences,Beijing 100190,China [3]Key Laboratory of Solar Activity and Space Weather,National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China [4]Hainan National Field Science Observation and Research Observatory for Space Weather,National Space Science Center,Chinese Academy of Sciences,Beijing 100190,China

出　　处：《Earth and Planetary Physics》2024年第4期632-640,共9页地球与行星物理（英文版）

基　　金：supported by the National Key R&D program of China(2021YFE0110200);the Project of Stable Support for Youth Team in Basic Research Field,CAS(YSBR-018);the National Natural Science Foundation of China(41831073,42174196 and 42174212);the Chinese Meridian Project;the Specialized Research Fund for State Key Laboratories;the International Partnership Program of Chinese Academy of Sciences.Grant No.183311KYSB20200003.

摘　　要：This study employs a linear inversion algorithm to retrieve volume emission rates(VERs)of molecular O_(2) nightglow at 1.27μm,utilizing Limb-Viewed spectra obtained from the SCanning Imaging Absorption spectroMeter for Atmospheric for CHartographY(SCIAMACHY)payload on board the Envisat satellite.The retrieved results are compared with VERs data from the SABER payload on the Thermosphere Ionosphere Mesosphere Energetics and Dynamics(TIMED)satellite,exhibiting consistency.This will help to facilitate accurate revelation of spatial distribution and periodic variation in O_(2) nightglow.VERs are extracted monthly within the altitude range of 75-110 km from 2002 to 2012,yielding a climatology of spatial and temporal distributions.The meridional structure exhibits two maxima,at the equator and at 45°N.Between August and October,the VERs exhibit a meridional bimodal structure,with the weaker one above the equator and the stronger one above 45°N.In April,the VERs reach their annual maximum.Additionally,harmonic analysis reveals significant temporal variations on different scales.The emission shows characteristics of annual and semi-annual variation,and a non-linear long-term trend associated with solar cycle activity.

关 键 词：VERs O_(2)1.27μm nightglow SCIAMACHY 

分 类 号：P407[天文地球—大气科学及气象学]