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首页> 外文期刊>Atmospheric Measurement Techniques >A reassessment of the discrepancies in the annual variation of delta D-H2O in the tropical lower stratosphere between the MIPAS and ACE-FTS satellite data sets
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A reassessment of the discrepancies in the annual variation of delta D-H2O in the tropical lower stratosphere between the MIPAS and ACE-FTS satellite data sets

机译:重新评估MIPA和ACE-FTS卫星数据集之间的热带较低平流层中DELTA D-H2O年度变化的差异

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The annual variation of delta D in the tropical lower stratosphere is a critical indicator for the relative importance of different processes contributing to the transport of water vapour through the cold tropical tropopause region into the stratosphere. Distinct observational discrepancies of the delta D annual variation were visible in the works of Steinwagner et al. (2010) and Randel et al. (2012). Steinwagner et al. (2010) analysed MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) observations retrieved with the IMK/IAA (Institut fur Meteorologie und Klimaforschung in Karlsruhe, Germany, in collaboration with the Instituto de Astrofisica de Andalucia in Granada, Spain) processor, while Randel et al. (2012) focused on ACE-FTS (Atmospheric Chemistry Experiment Fourier Transform Spectrometer) observations. Here we reassess the discrepancies based on newer MIPAS (IMK/IAA) and ACE-FTS data sets, also showing for completeness results from SMR (Sub-Millimetre Radiometer) observations and a ECHAM/MESSy (European Centre for Medium-Range Weather Forecasts Hamburg and Modular Earth Sub-model System) Atmospheric Chemistry (EMAC) simulation (Eichinger et al., 2015b). Similar to the old analyses, the MIPAS data set yields a pronounced annual variation (maximum about 75 parts per thousand), while that derived from the ACE-FTS data set is rather weak (maximum about 25 parts per thousand). While all data sets exhibit the phase progression typical for the tape recorder, the annual maximum in the ACE-FTS data set precedes that in the MIPAS data set by 2 to 3 months. We critically consider several possible reasons for the observed discrepancies, focusing primarily on the MIPAS data set. We show that the delta D annual variation in the MIPAS data up to an altitude of 40 hPa is substantially impacted by a "start altitude effect", i.e. dependency between the lowermost altitude where MIPAS retrievals are possible and retrieved data at higher altitudes. In itself this effect does not explain the differences with the ACE-FTS data. In addition, there is a mismatch in the vertical resolution of the MIPAS HDO and H2O data (being consistently better for HDO), which actually results in an artificial tape-recorder-like signal in delta D. Considering these MIPAS characteristics largely removes any discrepancies between the MIPAS and ACE-FTS data sets and shows that the MIPAS data are consistent with a delta D tape recorder signal with an amplitude of about 25 parts per thousand in the lowermost stratosphere.
机译:热带较低平流层中的ΔD的年度变化是不同过程对水蒸气通过冷热热带对流层次区域传输到平流层的不同过程的重要指标。斯坦瓦尔等人的作品可见三角洲二期变异的独特观察差异。 (2010)和兰德尔等人。 (2012)。 Steinwagner等。 (2010)分析了MIPAS(Michelson干涉仪为被动大气发出声音)与IMK / IAA(Institut Fur Meteorologie und Klimaforschung)与德国卡尔斯鲁厄的Institut de Astrofisica de Andalofia在格拉纳达,西班牙,西班牙,而且al。 (2012)专注于ACE-FTS(大气化学实验傅立叶变换光谱仪)观察。在这里,我们重新评估了基于较新的MIPAS(IMK / IAA)和ACE-FTS数据集的差异,也显示了SMR(亚毫米辐射计)观察和ECHAM /凌乱的完整性结果(欧洲的中等范围天气预报中心汉堡和模块化地球子模型系统)大气化学(EMAC)仿真(Eichinger等,2015b)。与旧分析类似,MIPAS数据集产生明显的年度变化(最大约75分),而源自ACE-FTS数据集相当弱(最大约为25分)。虽然所有数据集都表现出典型的磁带录音机的阶段进展,但ACE-FTS数据集中的年度最大值在MIPA数据中设置为2到3个月。我们批判地考虑了观察到的差异的几种可能的原因,主要关注MIPA数据集。我们表明,MIPA数据的Δd达到40hPa的高度的年度变化基本上受到“启动高度效应”的影响,即最下一度的依赖性,其中MIPAS检索是可能的并且在较高海拔地检索数据。本身本身不会解释与ACE-FTS数据的差异。另外,MIPA HDO和H2O数据的垂直分辨率存在不匹配(始终如一的HDO),其实际上导致ΔD中的人工带式卡录制的信号。考虑这些MIPAS特性在很大程度上消除了任何差异在MIPAS和ACE-FTS数据集之间,并表明MIPA数据与最下层平流层中每千幅幅度约为25份的Delta D录音机信号。

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