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首页> 外文期刊>Journal of Geophysical Research, D. Atmospheres: JGR >Retrieval of ozone and nitrogen dioxide concentrations from Stratospheric Aerosol and Gas Experiment III (SAGE III) measurements using a new algorithm
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Retrieval of ozone and nitrogen dioxide concentrations from Stratospheric Aerosol and Gas Experiment III (SAGE III) measurements using a new algorithm

机译:使用新算法从平流层气溶胶和气体实验III(SAGE III)测量中检索臭氧和二氧化氮浓度

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We describe a new inversion algorithm developed for the retrieval of atmospheric constituents from Stratospheric Aerosol and Gas Experiment III (SAGE III) solar occultation measurements. The methodology differs from the operational (NASA) algorithm in several important ways. Our algorithm takes account of the finite altitude and spectral resolution of the measurements by integrating over the viewing window spectrally and spatially. We solve the problem nonlinearly by using optimal estimation theory, and we use an aerosol parameterization scheme based on eigenvectors derived from existing empirical and modeled information about their microphysical properties. The first four of these eigenvectors are employed in the retrieval algorithm to describe the spectral variation of the aerosol extinction. We retrieve ozone and nitrogen dioxide number densities and aerosol extinction from transmission measurements at 41 channels from 0.29 to 1.55 μm. In this paper we describe the results of the gas retrievals. Numerical simulations test the accuracy of the scheme, and subsequent retrievals from SAGE III transmission data for the period between May and October 2002 produce profiles of O3 and NO2. Comparisons of the O3 and NO2 profiles with those obtained using the SAGE III operational algorithm and with those from independent measurements made by satellites, ozonesondes, and lidar indicate agreement in ozone measurements in the middle and upper stratosphere significantly closer than the natural variability and agreement in the lower stratosphere and upper troposphere approximately equal to the natural variability.
机译:我们描述了一种新的反演算法,该算法用于从平流层气溶胶和气体实验III(SAGE III)太阳掩星测量中检索大气成分。该方法在几个重要方面与可操作(NASA)算法不同。我们的算法通过在观察窗上进行光谱和空间积分来考虑测量的有限高度和光谱分辨率。我们通过使用最佳估计理论来非线性解决该问题,并使用基于特征向量的气溶胶参数化方案,该特征向量来自有关它们的微物理特性的现有经验和模型信息。这些特征向量的前四个在检索算法中用于描述气溶胶消光的光谱变化。我们从0.29到1.55μm的41个通道的透射测量结果中获取了臭氧和二氧化氮的数量密度和气溶胶的消灭。在本文中,我们描述了天然气回收的结果。数值模拟测试了该方案的准确性,随后在2002年5月至2002年10月期间从SAGE III传输数据中检索出O3和NO2的曲线。 O3和NO2剖面与使用SAGE III运算算法获得的剖面以及卫星,臭氧探空仪和激光雷达的独立测量所得的剖面相比,表明平流层中层和上方平流层中臭氧测量的一致性比自然变化和一致性更接近平流层下部和对流层上部大约等于自然变化率。

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