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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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MIPAS-ENVISAT full resolution spectra were analyzed to obtain a globaldistribution of hydrogen peroxide (H2O2) in the stratosphere.H2O2 acts as reservoir gas for the HOx family (= H+OH+HO2)and thus, observations of H2O2 provide a better understanding of theHOx chemistry in the atmosphere. A retrieval approach based onconstrained least squares fitting was developed and applied to smalldedicated spectral analysis windows with maximum H2O2 information andminimum contribution of interfering gases. Due to a low signal to noise ratioin the measured spectra single profiles cannot be used for scientificinterpretation and about 100 profiles have to be averaged temporally orspatially. Our retrievals of H2O2 from MIPAS measurements providemeaningful results between approximately 20 and 60 km. A possible impact bythe high uncertainty of the reaction rate constant forHO2 + HO2→H2O2 + O2 in our 3D-CTM KASIMA isdiscussed. We find best agreement between model and observations for applyingrate constants according to Christensen et al. (2002) however, a mismatch invertical profile shape remains. The observations were compared to the modelresults of KASIMA focusing on low to mid latitudes. Good agreement in spatialdistribution and in temporal evolution was found. Highest vmr of H2O2in the stratosphere were observed and modeled in low latitudes shortly afterequinox at about 30 km. The modelled diurnal cycle with lowest vmr shortlyafter sunrise and highest vmr in the afternoon is confirmed by the MIPASobservations.
机译:分析了MIPAS-ENVISAT全分辨率光谱,获得了平流层中过氧化氢(H 2 O 2 )的全球分布.H 2 O < sub> 2 充当HO x 族(= H + OH + HO 2 )的储层气,因此对H 2 < / sub> O 2 可更好地了解大气中HO x 的化学性质。提出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 2 O 2 信息和最小干扰气体贡献的小型专用光谱分析窗口。由于测得的频谱中信噪比低,因此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 2 O 2 提供了大约20至60 km之间有意义的结果。 HO 2 + HO 2 →H 2 O 2 +的反应速率常数的高度不确定性可能产生影响讨论了我们3D-CTM KASIMA中的O 2 。根据Christensen等人的研究,我们发现模型和观测值之间的最佳一致性适用于速率常数。 (2002年),但不匹配的垂直轮廓形状仍然存在。将这些观察结果与KASIMA的模型结果进行了比较,该模型结果侧重于中低纬度。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处的低纬度观测到平流层中H 2 O 2 的最高vmr并进行建模。 MIPAS观测证实了模拟的昼夜周期,其日出后不久的vmr最低,下午的vmr最高。

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