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首页> 外文期刊>Atmospheric chemistry and physics >Global stratospheric hydrogen peroxide distribution from MIPAS-Envisat full resolution spectra compared to KASIMA model results
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Global stratospheric hydrogen peroxide distribution from MIPAS-Envisat full resolution spectra compared to KASIMA model results

机译:来自MIPAS-Envisat全分辨率光谱的全球平流层过氧化氢分布与KASIMA模型结果相比

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摘要

MIPAS-ENVISAT full resolution spectra were analyzed to obtain a global distribution of hydrogen peroxide (H _2O _2) in the stratosphere. H _2O _2 acts as reservoir gas for the HOx family (Combining double low line H+OH+HO2) and thus, observations of H _2O _2 provide a better understanding of the HOx chemistry in the atmosphere. A retrieval approach based on constrained least squares fitting was developed and applied to small dedicated spectral analysis windows with maximum H _2O _2 information and minimum contribution of interfering gases. Due to a low signal to noise ratio in the measured spectra single profiles cannot be used for scientific interpretation and about 100 profiles have to be averaged temporally or spatially. Our retrievals of H _2O _2 from MIPAS measurements provide meaningful results between approximately 20 and 60 km. A possible impact by the high uncertainty of the reaction rate constant for HO2 +HO _2→H _2O _2 +O _2in our 3D-CTM KASIMA is discussed. We find best agreement between model and observations for applying rate constants according to Christensen et al. (2002) however, a mismatch in vertical profile shape remains. The observations were compared to the model results of KASIMA focusing on low to mid latitudes. Good agreement in spatial distribution and in temporal evolution was found. Highest vmr of H _2O _2 in the stratosphere were observed and modeled in low latitudes shortly after equinox at about 30 km. The modelled diurnal cycle with lowest vmr shortly after sunrise and highest vmr in the afternoon is confirmed by the MIPAS observations.
机译:分析了MIPAS-ENVISAT的全分辨率光谱,以获得平流层中过氧化氢(H _2O _2)的全局分布。 H _2O _2充当HOx族的储气库(结合双低线H + OH + HO2),因此,对H _2O _2的观察可以更好地理解大气中的HOx。开发了一种基于约束最小二乘拟合的检索方法,并将其应用于具有最大H _2O _2信息和最小干扰气体贡献的小型专用光谱分析窗口。由于测得的光谱中信噪比低,无法将单个配置文件用于科学解释,并且必须在时间或空间上平均约100个配置文件。我们从MIPAS测量中获得的H _2O _2提供了大约20至60 km之间的有意义的结果。讨论了在我们的3D-CTM KASIMA中,HO2 + HO _2→H _2O _2 + O _2的反应速率常数的高度不确定性可能产生的影响。我们发现,根据Christensen等人的方法,在应用速率常数的模型和观测值之间可以找到最佳的一致性。 (2002年),但垂直轮廓形状不匹配仍然存在。将这些观察结果与KASIMA的模型结果(重点放在中低纬度)进行了比较。发现在空间分布和时间演变方面有很好的一致性。在平流层后约30 km处,在低纬度观测到平流层中H _2O _2的最高vmr并进行建模。 MIPAS的观测结果证实了模型化的昼夜周期,日出后不久vmr最低,下午vmr最高。

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