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首页> 外文期刊>Atmospheric chemistry and physics >Combined SAGE II–GOMOS ozone profile data set for 1984–2011 and trend analysis of the vertical distribution of ozone
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Combined SAGE II–GOMOS ozone profile data set for 1984–2011 and trend analysis of the vertical distribution of ozone

机译:结合1984年至2011年的SAGE II–GOMOS臭氧剖面数据集和臭氧垂直分布的趋势分析

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摘要

We have studied data from two satellite occultation instruments in order togenerate a high vertical resolution homogeneous ozone time series of 26 yr. The Stratospheric Aerosol and Gas Experiment (SAGE) II solaroccultation instrument and the Global Ozone Monitoring byOccultation of Stars (GOMOS) instrument measured ozoneprofiles in the stratosphere and mesosphere from 1984–2005 and 2002–2012, respectively. Global coverage, good verticalresolution, and the self-calibrating measurement method make data from theseinstruments valuable for the detection of changes in vertical distribution ofozone over time. As both instruments share a common measurement period from2002–2005, it is possible to inter-calibrate the data sets. We investigatehow well these measurements agree with each other and combine all the data toproduce a new stratospheric ozone profile data set. Above 55 km, SAGE IImeasurements show much less ozone than the GOMOS nighttime measurements as aconsequence of the well-known diurnal variation of ozone in the mesosphere.Between 35–55 km, SAGE II sunrise and sunset measurements differ from GOMOS' measurements to different extents. Sunrise measurements show 2% less ozone than GOMOS, whereas sunsetmeasurements show 4% more ozone than GOMOS. Differences can be explainedqualitatively by the diurnal variation of ozone in the stratosphere recentlyobserved by SMILES and modeled by chemical transport models. Between 25–35 km, SAGE II sunrise and sunset measurements and GOMOS measurements agree within 1%.The observed ozone bias between collocated measurements of SAGE IIsunrise/sunset and GOMOS night measurements is used to align the two datasets. The combined data set covers the time period 1984–2011, latitudes60° S–60° N, and the altitude range of 20–60 km. Profile data aregiven on a 1 km vertical grid, and with a resolution of 1 month in time and10° in latitude. The combined ozone data set is analyzed by fitting atime series model to the data. We assume a linear trend with an inflectionpoint (so-called "hockey stick" form). The best estimate for the point ofinflection was found to be the year 1997 for ozone between altitudes 35 and45 km. At all latitudes and altitudes from 35 to 50 km we find a clearchange in ozone trend before and after the inflection time. From 38 to 45km, a negative trend of 4% per decade (statistically significant at 95%level) at the equator has changed to a small positive trend of 0–2% perdecade. At mid-latitudes, the negative trend of 4–8% per decade has changedto to a small positive trend of 0–2% per decade. At mid-latitudes near 20 km, the ozone loss has still increased whereas in the tropics a recovery is ongoing.
机译:我们已经研究了来自两种卫星掩星仪器的数据,以便产生26年的高垂直分辨率均匀臭氧时间序列。平流层气溶胶和天然气实验(SAGE)II太阳掩星仪和全球星际掩星监测臭氧(GOMOS)仪分别测量了1984-2005年和2002-2012年平流层和中层的臭氧分布。全球覆盖率,良好的垂直分辨率和自校准测量方法使这些仪器的数据对于检测臭氧随时间的垂直分布变化具有重要价值。由于这两种仪器在2002年至2005年之间共有一个共同的测量期间,因此可以对数据集进行相互校准。我们调查了这些测量之间的吻合程度,并结合了所有数据以产生一个新的平流层臭氧剖面数据集。在55公里以上,SAGE II测量显示的臭氧量比GOMOS夜间测量的臭氧量少得多,这是由于已知中层臭氧的昼夜变化所致。在35-55 km之间,SAGE II日出和日落测量与GOMOS的测量有所不同。日出测量显示的臭氧量比GOMOS少2%,而日落测量显示的臭氧量比GOMOS多4%。 SMILES最近观测到的平流层中臭氧的昼夜变化可以用定性的方法解释,并可以通过化学迁移模型进行模拟。在25-35公里之间,SAGE II日出和日落测量值与GOMOS测量值相吻合在1%以内。 在SAGE II日出/日落并置测量值与GOMOS夜间测量值并存的测量值中观察到的臭氧偏差用于对齐两个数据集。组合的数据集涵盖了1984-2011年的时间段,北纬60°S-60°N和20-60 km的海拔范围。纵断面数据在1 km的垂直网格上给出,分辨率为1个月,纬度为10°。通过对数据拟合时间序列模型来分析合并的臭氧数据集。我们假设一个带有拐点的线性趋势(所谓的“曲棍球棒”形式)。发现拐点的最佳估计是1997年海拔35至45公里之间的臭氧。在35至50 km的所有纬度和海拔上,我们都发现了在拐弯前后的臭氧趋势发生了明显变化。从38 km到45 km,赤道每10年出现4%的负趋势(在95%的水平上具有统计意义),已变成每十年10%至2%的小正趋势。在中纬度地区,每十年4-8%的负趋势已变为每十年0-2%的小正趋势。在接近20公里的中纬度地区,臭氧的损失仍在增加,而在热带地区,臭氧的恢复仍在继续。

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