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稳定场大气层顶反射率模型光谱拓展方法及不确定性分析

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基于稳定场的辐射定标利用大气层顶(TOA)反射率模型,直接计算入瞳辐亮度而无需地面同步测量,能够实现光学遥感载荷的高频次辐射定标。针对当前国内陆表稳定场的通道式TOA反射率模型在光谱分辨率上的局限性,提出一种针对稳定场TOA通道式反射率模型的光谱拓展方法,引入GF5B/AHSI卫星高光谱数据提取参考光谱,与稳定场TOA通道式反射率联合求解光谱缩放因子,实现TOA通道式反射率模型在光谱维度上的拓展,所构建的稳定场TOA反射率光谱模型适用于光谱响应各异的不同卫星光学载荷的绝对辐射定标。进一步利用Sentinel2/MSI和Landsat8/OLI卫星数据对稳定场TOA反射率光谱模型进行验证,并基于GF6/WFV卫星的定标过程给出绝对辐射定标结果的不确定度分析。结果表明:模型预测值和Sentinel2/MSI、Landsat8/OLI观测值的平均相对误差在±5%以内,GF6/WFV的8个波段定标不确定度小于5。4%,充分证明所构建光谱拓展模型的有效性。
A Method for Hyperspectral Reflectance Expansion from Multispectral Reflectance Model of Stable Sites and Uncertainty Analysis
Objective The radiometric calibration based on pseudo-invariant calibration site(PICS)can calculate the apparent radiance directly by using the reflectance model of top of atmosphere(TOA)established by high precision remote sensing sensors without ground synchronous observation.This enables high precision and high frequency radiometric calibration of optical remote sensing sensors.Currently,the trend in radiometric calibration based on PICS is to relax the stability constraints of the surface and atmosphere to increase the number of stable sites,thereby obtaining more satellite transit frequency and achieving higher frequency on-orbit radiometric calibration.However,current multispectral models can only predict the TOA reflectance of a few channels,limiting the use of the stable site model.In this paper,we present a method for hyperspectral reflectance expansion from multispectral reflectance,which realizes the expansion of the existing multispectral model in spectral dimension.We construct the TOA hyperspectral reflectance model of the East of Dazaohuo stable sites and the West of Xiao Qaidam Lake stable sites.Compared with the multispectral model,the precision of the TOA hyperspectral reflectance model in the original five channels is not significantly reduced and can provide on-orbit radiometric calibration service for optical sensors in transit of 400-2500 nm.Methods The GF5B/AHSI is a hyperspectral sensor with 330 imaging channels covering the 400-2500 nm band range,and its historical spectrum over the stable sites remains stable(Fig.2).In our paper,the mean value of its historical data is selected as the reference TOA reflectivity spectrum.Assuming a linear relationship between the ratio of TOA hyperspectral reflectance to its corresponding channel reflectance,the reference spectrum is normalized to the spectral responses of moderate-resolution imaging spectroradiometer(MODIS)as equivalent channel reflectance to have a uniform scale within the model.Subsequently,information on solar attitude,observation attitude and day of year(DOY)is extracted,and the channel TOA reflectance over the transit stable sites is predicted by the multispectral model.Then,the ratio of TOA channel reflectance to equivalent channel reflectance during satellite transit is calculated,linearly interpolated across the spectral band as a spectral scaling factor,and applied to scale the reference spectrum.This process realizes the spectral dimension expansion of the model and constructs the TOA hyperspectral reflectance model of the stable sites.Results and Discussions Landsat8/OLI data from 2013 to 2021 and Sentinel2/MSI data from 2018 to 2021 are used to verify the proposed method.The results show an average relative difference between the model's predicted values and the satellite's observed values of no more than±4%,with a root mean square error(RMSE)of each band of no more than 1.5%(Table 2,Table 3).Compared with the TOA multispectral model,the average relative difference of the blue wave segment based on Sentinel2/MSI data increases from-1.02%to-1.61%,and the RMSE from 0.36%to 0.42%.The average relative difference of the shortwave infrared band increases from-0.12%to-0.94%,and the RMSE from 0.61%to 0.68%.The precision of the other three bands is consistent with that of the multispectral model,indicating that the precision of the method in the original several channels is not significantly reduced.At the West of the Xiao Qaidam Lake site,the average relative difference between the model-predicted value and the satellite-observed value is less than±3.1%,with an RMSE for each band of less than 1.1%(Table 6,Table 7).The verification results of the two stable site models show that the predicted values of TOA hyperspectral reflectance of the stable sites maintain high consistency with the satellite observation values.Meanwhile,the model also analyzes the uncertainty of the calibration result based on the calibration process of GF6/WFV sensors.The uncertainty of eight bands of GF6/WFV is less than 4.5%,which is 0.49%lower than the average uncertainty of the original multispectral reflectance model.Conclusions In this paper,we present a method for hyperspectral reflectance expansion from multispectral reflectance,utilizing the mean value of GF5B/AHSI data as the reference spectrum and normalizing it to the MODIS spectral response as equivalent channel reflectance.The channel TOA reflectance over the transit stable sites is predicted by the multispectral model.Then,the ratio of TOA channel reflectance to equivalent channel reflectance during satellite transit is calculated,and the ratio is linearly interpolated across the spectral band as a spectral scaling factor.This factor is then used to scale the reference spectrum,realizing the spectral dimension expansion of the model.In our study,Sentinel2/MSI data and Landsat8/OLI data are used to evaluate the precision of the East of Dazaohuo and West of Xiao Qaidam Lake sites.The results demonstrate high agreement between the model's predicted values and satellite observation values.The precision across each band of the model is similar,indicating that the model's precision itself can remain stable.Based on the calibration process of GF6/WFV sensors,an uncertainty analysis of model calibration results is conducted.The uncertainty of eight bands of GF6/WFV sensors is less than 5.4%,further verifying the reliability of the model.The uncertainty analysis of the calibration results helps characterize the uncertainty of the calibration results and ensures consistency and traceability of satellite sensors calibration results.In future studies,the TOA hyperspectral reflectance model can also generate time series calibration results for satellite sensors,providing long-term trend information for individual sensors.Moreover,based on multiple stable site models,multi-site calibrations can also be performed to further improve the on-orbit calibration frequency of sensors,which is significantly important for the commercial calibration of domestic satellite sensors.

radiometric calibrationstable site modeltop of atmosphere reflectancespectral expansionuncertainty analysis

鲁鑫、赵永光、马灵玲、王宁、韩启金、陶醉、赵江洪、李婉、王任飞、张栩源

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中国科学院空天信息创新研究院遥感卫星应用国家工程实验室,北京 100094

中国科学院大学电子电气与通信工程学院,北京 100049

中国资源卫星应用中心,北京 100094

北京建筑大学测绘与城市空间信息学院,北京 100044

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辐射定标 稳定场模型 大气层顶反射率 光谱拓展 不确定性分析

2024

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCD北大核心
影响因子:1.931
ISSN:0253-2239
年,卷(期):2024.44(24)