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Combined SAGE IIa??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 IIa ?? GOMOS臭氧剖面数据集和臭氧垂直分布的趋势分析

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pstrongAbstract./strong We have studied data from two satellite occultation instruments in order to generate a high vertical resolution homogeneous ozone time series of 26 yr. The Stratospheric Aerosol and Gas Experiment (SAGE) II solar occultation instrument and the Global Ozone Monitoring by Occultation of Stars (GOMOS) instrument measured ozone profiles in the stratosphere and mesosphere from 1984a??2005 and 2002a??2012, respectively. Global coverage, good vertical resolution, and the self-calibrating measurement method make data from these instruments valuable for the detection of changes in vertical distribution of ozone over time. As both instruments share a common measurement period from 2002a??2005, it is possible to inter-calibrate the data sets. We investigate how well these measurements agree with each other and combine all the data to produce a new stratospheric ozone profile data set. Above 55 km, SAGE II measurements show much less ozone than the GOMOS nighttime measurements as a consequence of the well-known diurnal variation of ozone in the mesosphere. Between 35a??55 km, SAGE II sunrise and sunset measurements differ from GOMOS' measurements to different extents. Sunrise measurements show 2% less ozone than GOMOS, whereas sunset measurements show 4% more ozone than GOMOS. Differences can be explained qualitatively by the diurnal variation of ozone in the stratosphere recently observed by SMILES and modeled by chemical transport models. Between 25a??35 km, SAGE II sunrise and sunset measurements and GOMOS measurements agree within 1%. brbr The observed ozone bias between collocated measurements of SAGE II sunrise/sunset and GOMOS night measurements is used to align the two data sets. The combined data set covers the time period 1984a??2011, latitudes 60?° Sa??60?° N, and the altitude range of 20a??60 km. Profile data are given on a 1 km vertical grid, and with a resolution of 1 month in time and 10?° in latitude. The combined ozone data set is analyzed by fitting a time series model to the data. We assume a linear trend with an inflection point (so-called "hockey stick" form). The best estimate for the point of inflection was found to be the year 1997 for ozone between altitudes 35 and 45 km. At all latitudes and altitudes from 35 to 50 km we find a clear change in ozone trend before and after the inflection time. From 38 to 45 km, a negative trend of 4% per decade (statistically significant at 95% level) at the equator has changed to a small positive trend of 0a??2% per decade. At mid-latitudes, the negative trend of 4a??8% per decade has changed to to a small positive trend of 0a??2% per decade. At mid-latitudes near 20 km, the ozone loss has still increased whereas in the tropics a recovery is ongoing./p.
机译:> >摘要。我们研究了来自两种卫星掩星仪器的数据,以生成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仪(GOMOS)分别测量了1984a-2005年和2002a-2012年平流层和中层的臭氧分布。全球覆盖范围,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。由于这两种仪器共有一个从2002a至2005年的共同测量期间,因此可以对数据集进行相互校准。我们调查了这些测量结果相互之间的吻合程度,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,由于众所周知的中层臭氧的昼夜变化,SAGE II测得的臭氧比GOMOS夜间测得的少得多。在35a?55 km之间,SAGE II日出和日落测量值与GOMOS的测量值有所不同。日出测量值显示的臭氧量比GOMOS少2%,而日落测量值显示的臭氧量比GOMOS多4%。可以通过SMILES最近观测到的平流层中臭氧的昼夜变化定性地解释这种差异,并通过化学迁移模型进行建模。在25a?35 km之间,SAGE II日出和日落测量值与GOMOS测量值相差1%。 在SAGE II日出/日落和GOMOS夜间测量的并置测量之间观察到的臭氧偏差用于对齐两个数据集。合并的数据集涵盖时间段1984a ?? 2011,纬度60?Sa Sa?60?N和20a?60 km的海拔范围。剖面资料是在1 km的垂直网格上给出的,分辨率为1个月,纬度为10°。通过将时间序列模型拟合到数据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时间前后臭氧趋势的明显变化。从38 km到45 km,赤道每10年出现4%的负趋势(在95%的水平上具有统计学意义)已变为每10年0a ?? 2%的小正趋势。在中纬度地区,每十年负4a 8%的负趋势已变为每十年负aa 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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