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The Antarctic Oscillation Structure in an AOGCM with Interactive Stratospheric Ozone

机译:带有平流层臭氧相互作用的AOGCM中的南极振荡结构

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Based on 150-year equilibrium simulations using the atmosphere-ocean-sea ice general circulation model (AOGCM) ECHO-GiSP, the southern hemisphere winter circulation is examined focusing on tropo-stratosphere coupling and wave dynamics. The model covers the troposphere and strato-mesosphere up to 80 km height and includes an interactive stratospheric chemistry. Compared to the reference simulation without interactive chemistry, the interactive simulation shows a weaker polar vortex in the middle atmosphere and is shifted towards the negative phase of the Antarctic Oscillation (AAO) in the troposphere. Differing from the northern hemisphere winter situation, the tropospheric planetary wave activity is weakened. A detailed analysis shows, that the modelled AAO zonal mean signal behaves antisymmetrically between troposphere and strato-mesosphere. This conclusion is supported by reanalysis data and a discussion of planetary wave dynamics in terms of Eliassen-Palm fluxes. Thereby, the tropospheric planetary wave activity appears to be controlled from the middle atmosphere.
机译:基于使用大气-海洋-海冰总循环模型(AOGCM)ECHO-GiSP进行的150年平衡模拟,对南半球冬季循环进行了研究,重点是对流层-平流层耦合和波浪动力学。该模型覆盖了高达80 km高度的对流层和平流-中流层,并包括一个互动的平流层化学物质。与没有交互化学作用的参考模拟相比,交互模拟在中层大气中显示出更弱的极涡,并向对流层中的南极涛动(AAO)的负相移动。与北半球冬季不同,对流层行星波活动减弱。详细分析表明,模拟的AAO纬向平均信号在对流层与平流-中层之间呈反对称表现。这一结论得到了再分析数据的支持,并根据Eliassen-Palm通量讨论了行星波动力学。因此,对流层行星波活动似乎是由中间大气控制的。

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