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DOI | 10.5194/acp-20-281-2020 |
Attribution of Chemistry-Climate Model Initiative (CCMI) ozone radiative flux bias from satellites | |
Kuai L.; Bowman K.W.; Miyazaki K.; Deushi M.; Revell L.; Rozanov E.; Paulot F.; Strode S.; Conley A.; Jöckel P.; Plummer D.A.; Oman L.D.; Worden H.; Kulawik S.; Paynter D.; Stenke A.; Kunze M. | |
发表日期 | 2020 |
ISSN | 16807316 |
起始页码 | 281 |
结束页码 | 301 |
卷号 | 20期号:1 |
英文摘要 | The top-of-atmosphere (TOA) outgoing longwave flux over the 9.6 μm ozone band is a fundamental quantity for understanding chemistry-climate coupling. However, observed TOA fluxes are hard to estimate as they exhibit considerable variability in space and time that depend on the distributions of clouds, ozone (O3), water vapor (H2O), air temperature (Ta), and surface temperature (Ts). Benchmarking present-day fluxes and quantifying the relative influence of their drivers is the first step for estimating climate feedbacks from ozone radiative forcing and predicting radiative forcing evolution. To that end, we constructed observational instantaneous radiative kernels (IRKs) under clear-sky conditions, representing the sensitivities of the TOA flux in the 9.6 μm ozone band to the vertical distribution of geophysical variables, including O3, H2O, Ta, and Ts based upon the Aura Tropospheric Emission Spectrometer (TES) measurements. Applying these kernels to present-day simulations from the Chemistry-Climate Model Initiative (CCMI) project as compared to a 2006 reanalysis assimilating satellite observations, we show that the models have large differences in TOA flux, attributable to different geophysical variables. In particular, model simulations continue to diverge from observations in the tropics, as reported in previous studies of the Atmospheric Chemistry Climate Model Intercomparison Project (ACCMIP) simulations. The principal culprits are tropical middle and upper tropospheric ozone followed by tropical lower tropospheric H2O. Five models out of the eight studied here have TOA flux biases exceeding 100 mW m-2 attributable to tropospheric ozone bias. Another set of five models have flux biases over 50 mW m-2 due to H2O. On the other hand, Ta radiative bias is negligible in all models (no more than 30 mW m-2). We found that the atmospheric component (AM3) of the Geophysical Fluid Dynamics Laboratory (GFDL) general circulation model and Canadian Middle Atmosphere Model (CMAM) have the lowest TOA flux biases globally but are a result of cancellation of opposite biases due to different processes. Overall, the multi-model ensemble mean bias is |
关键词 | air temperatureatmospheric chemistryatmospheric modelingclimate feedbackclimate modelinglongwave radiationozoneradiative forcingsatellite imagerysurface temperature |
语种 | 英语 |
来源机构 | Atmospheric Chemistry and Physics |
文献类型 | 期刊论文 |
条目标识符 | http://gcip.llas.ac.cn/handle/2XKMVOVA/132312 |
推荐引用方式 GB/T 7714 | Kuai L.,Bowman K.W.,Miyazaki K.,et al. Attribution of Chemistry-Climate Model Initiative (CCMI) ozone radiative flux bias from satellites[J]. Atmospheric Chemistry and Physics,2020,20(1). |
APA | Kuai L..,Bowman K.W..,Miyazaki K..,Deushi M..,Revell L..,...&Kunze M..(2020).Attribution of Chemistry-Climate Model Initiative (CCMI) ozone radiative flux bias from satellites.,20(1). |
MLA | Kuai L.,et al."Attribution of Chemistry-Climate Model Initiative (CCMI) ozone radiative flux bias from satellites".20.1(2020). |
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