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1.27μmO2(a1Δg)气辉临边观测辐射传输特性

Radiative Transfer Characteristics of the 1.27 μm O2(a1Δg)Airglow in Limb-Viewing

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1.27μm波段的O2(a1 Δg)气辉辐射具有辐射信号强、空间跨度大、自吸收效应弱等诸多内禀优势,是临近空间大气遥感的重要目标源,对于中高层大气的动力学及热学特性研究,全球温室气体探测,以及臭氧浓度三维层析等卫星遥感具有重要的科学意义和应用价值.首先基于O2(a1 Δg)光化学反应模型,研究了02(a1Δg)气辉的产生机制及湮灭机理,在此基础上,计算得到了 O2(a1 Δg)气辉体辐射率廓线,并基于HIT-RAN数据库给出的谱线强度及爱因斯坦系数,提出了两种计算O2(a1 Δg)气辉光谱分布的方法.采用最新的分子光谱参数、光化学反应速率常数及F10.7太阳紫外通量等参数,结合光化学反应模型计算得到的O2(a1Δg)气辉体辐射率廓线信息,借助逐线积分算法,建立了 1.27μmO2(a1Δg)气辉临边观测辐射传输理论模型,并分析了自吸收效应对不同临边观测高度处气辉辐射光谱强度的影响.然后,利用剥洋葱算法,对大气图像扫描成像吸收光谱仪(SCIAMACHY)在临边观测模式下测得的O2分子近红外大气带的气辉辐射信号进行处理得到了目标层O2(a1Δg)气辉辐射光谱,并通过谱积分算法反演得到了 O2(a1Δg)气辉的体辐射率廓线信息.最后通过对比气辉临边观测辐射传输理论模型计算得到的以及SCIAMACHY仪器测量反演得到的1.27μmO2(a1 Δg)辐射光谱及体辐射率廓线信息,验证1.27μmO2(a1Δg)气辉临边观测辐射传输理论模型的可靠性与合理性.基于比对结果,对O2(a1Δg)气辉临边辐射强度和体辐射率的影响因素进行了分析.分析结果表明,在50 km以上的高空区域,理论计算结果与卫星实测结果吻合性较好,而随着海拔高度的降低,两者的偏差逐渐增大,这是因为在临边观测模式下,中低空区域的卫星遥感信号受自吸收效应及大气散射效应影响严重.此外,与HITRAN数据库给出的谱线强度参数相比,基于爱因斯坦系数建立的O2(a1 Δg)气辉临边辐射模型与卫星实测结果更加吻合.1.27μmO2(a1 Δg)气辉临边观测辐射传输理论模型的建立,对于临近空间大气遥感,奠定了理论基础.
Because the 1.27 μm O2(a1Δg)airglow radiation has the advantages of strong radiation signal,large space span and weak self-absorption effect,it is an important target source for near-space atmospheric remote sensing.In addition,it has important scientific significance and application value,such as research on the dynamics and thermal characteristics of the middle and upper atmosphere,global greenhouse gas detection,and three-dimensional tomography of ozone concentration.Firstly,based on the photochemical model of O2(a1 Δg),the generation and annihilation mechanisms of O2(a1Δg)airglow were studied.The volume emission rate profile of O2(a1 Δg)airglow was calculated on this basis.Based on the spectral intensity and Einstein coefficients given by HITRAN,two methods for calculating the spectral distribution of O2(a1 Δg)airglow were proposed.Using the latest molecular spectral parameters,photochemical reaction rate constant and F10.7 solar ultraviolet flux,combined with the volume emission rate profile information of O2(a1 Δg)airglow calculated by photochemical reaction model.The radiative transfer theoretical model of the 1.27 μm O2(a1Δg)airglow in limb-viewing was developed by using a line-by-line integration algorithm.The influence of the self-absorption effect on the spectral intensity of airglow radiation at different tangent heights is analyzed.Then,the O2(a1Δg)airglow radiation spectrum of the target layer is obtained by processing the airglow radiation of the O2 molecule near the infrared atmospheric band measured by scanning imaging absorption spectrometer for atmospheric chartography(SCIAMACHY)under the limb-viewing by onion peeling algorithm.Spectral integration algorithm is used to retrieve the volume emission rate profile of O2(a1 Δg)airglow.Finally,the reliability and rationality of the radiative transfer theoretical model of the 1.27 μm O2(a1 Δg)airglow in limb-viewing is verified by comparing the radiation spectrum and the volume emission rate profile obtained from the theoretical calculation and retrieval of the SCIAMACHY instrument.Regarding the comparison results,factors that contribute to the limb radiation intensity and volume emission rate of O2(a1Δg)airglow are analyzed.Analyses show that theoretical calculations agree with measured satellite results in the altitude region above 50 km.However,the deviation between the two increases gradually with the decrease of altitude because the satellite remote sensing in the middle and low altitude regions are seriously affected by the self-absorption effect and atmospheric scattering effect in limb-viewing.Additionally,compared with the spectral line intensity parameter given by the HITRAN database,the O2(a1Δg)airglow limb radiation model based on Einstein coefficients is more consistent with the measured satellite results.Establishing the radiative transfer theoretical model of the 1.27 μm O2(a1Δg)airglow in limb-viewing provides a theoretical foundation for atmospheric remote sensing in near space.

O2(a1 Δg)band airglowVolume emission rateLimb-viewingRadiative transfer theoretical model

王道琦、王后茂、何微微、胡向瑞、李娟、李发泉、武魁军

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烟台大学物理与电子信息学院,山东烟台 264005

中国科学院国家空间科学中心,北京 100190

中国科学院西安光学精密机械研究所,陕西西安 710119

中国科学院精密测量科学与技术创新研究院,湖北武汉 430071

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O2(a1Δg)气辉 体辐射率 临边观测 辐射传输理论模型

国家自然科学基金国家自然科学基金山东省高等学校青年创新技术项目山东省自然科学基金烟台大学研究生科研创新基金

41975039417041782021KJ008ZR2021QD088GGIFYTU2313

2024

光谱学与光谱分析
中国光学学会

光谱学与光谱分析

CSTPCD北大核心
影响因子:0.897
ISSN:1000-0593
年,卷(期):2024.44(4)
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