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Assessment of the quality of ACE-FTS stratospheric ozone data
Atmospheric Measurement Techniques ( IF 3.2 ) Pub Date : 2021-08-30 , DOI: 10.5194/amt-2021-252
Patrick E. Sheese , Kaley A. Walker , Chris D. Boone , Adam E. Bourassa , Doug A. Degenstein , Lucien Froidevaux , C. Thomas McElroy , Donal Murtagh , James M. Russell III , Jiansheng Zou

Abstract. For the past 17 years, the Atmospheric Chemistry Experiment Fourier Transform Spectrometer (ACE-FTS) instrument on the Canadian SCISAT satellite has been measuring profiles of atmospheric ozone. The latest two operational versions of the level 2 ozone data are versions 3.6 and 4.1. This technical note characterizes how both products compare with correlative data from other limb-sounding satellite instruments, namely MAESTRO, MLS, OSIRIS, SABER, and SMR. In general, v3.6, with respect to the other instruments, exhibits a smaller bias (which is on the order of ~3 %) in the middle stratosphere than v4.1 (~2–9 %), however the bias exhibited in the v4.1 data tends to be more stable, i.e. not changing significantly over time in any altitude region. In the lower stratosphere, v3.6 has a positive bias of about 3–5 % that is stable to within ±1 % dec−1, and v4.1 has a bias on the order of −1 to +5 % and is also stable to within ±1 % dec−1. In the middle stratosphere, v3.6 has a positive bias of ~3 % with a significant negative drift on the order of 0.5–2.5 % dec−1, and v4.1 has a positive bias of 2–9 % that is stable to within ±0.5 % dec−1. However, the v4.1 bias in the middle stratosphere is reduced to 0–5 % after being corrected for field-of-view modelling errors. In the upper stratosphere, v3.6 has a positive bias that increases with altitude up to ~16 % and a significant negative drift on the order of 2–3 % dec−1, and v4.1 has a positive bias that increases with altitude up to ~15 % and is stable to within ±1 % dec−1.

中文翻译:

ACE-FTS 平流层臭氧数据质量评估

摘要。在过去的 17 年中,加拿大 SCISAT 卫星上的大气化学实验傅里叶变换光谱仪 (ACE-FTS) 仪器一直在测量大气臭氧的轮廓。2 级臭氧数据的最新两个运行版本是版本 3.6 和 4.1。本技术说明描述了这两种产品如何与来自其他肢体探测卫星仪器(即 MAESTRO、MLS、OSIRIS、SABER 和 SMR)的相关数据进行比较。一般来说,相对于其他仪器,v3.6 在平流层中间表现出比 v4.1 (~2-9%) 更小的偏差(大约 ~3%),但是偏差在v4.1 数据往往更稳定,即在任何海拔区域都不会随时间发生显着变化。在平流层下层,v3.6 有大约 3-5% 的正偏差,稳定在 ±1% dec-1和 v4.1 具有 -1 到 +5 % 数量级的偏差,并且在 ±1 % dec -1范围内也稳定。在中间平流层,v3.6 有~3% 的正偏差,有 0.5-2.5% dec -1的显着负漂移,v4.1 有 2-9% 的正偏差,稳定到在±0.5 % dec -1 内。但是,经过视场建模错误校正后,平流层中部的 v4.1 偏差降低到 0-5%。在平流层上层,v3.6 有一个正偏差,随着海拔高度增加高达 ~16 % 和一个显着的负漂移大约 2–3 % dec -1,v4.1 有一个正偏差,随着海拔高度增加高达 ~15 % 并且稳定在 ±1 % dec -1以内。
更新日期:2021-08-30
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