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On the role of the planetary boundary layer depth in the climate system

机译:行星边界层深度在气候系统中的作用

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The planetary boundary layer (PBL) is a part of theEarth's atmosphere where turbulent fluxes dominate vertical mixing andconstitute an important part of the energy balance. The PBL depth, h, isrecognized as an important parameter, which controls some features of theEarth's climate and the atmospheric chemical composition. It is also knownthat h varies by two orders of magnitude on diurnal and seasonal timescales. This brief note highlights effects of this variability on theatmospheric near-surface climate and chemical composition. We interpret heatcapacity parameter of a Budyko-type energy balance model in terms ofquasi-equilibrium h. The analysis shows that it is the shallowest,stably-stratified PBL with the smallest h that should be of particularconcern for climate modelling. The reciprocal dependence between the PBLdepth and temperature (concentrations) is discussed. In particular, theanalysis suggests that the climate characteristics during stably stratifiedPBL episodes should be significantly more sensitive to perturbations of theEarth's energy balance as well as emission rates. On this platform, h fromERA-40 reanalysis data, the CHAMP satellite product and the DATABASE64 datawere compared. DATABASE64 was used to assess the Troen-Mahrt method todetermine h through available meteorological profile observations. As ithas been found before, the shallow PBL requires better parameterization andbetter retrieval algorithms. The study demonstrated that ERA-40 and CHAMPdata are biased toward deeper h in the shallow polar PBL. This, coupledwith the scarcity of in-situ observations might mislead the attribution ofthe origins of the Arctic climate change mechanisms.
机译:行星边界层(PBL)是地球大气的一部分,湍流在垂直混合中占主导地位,是能量平衡的重要组成部分。 PBL深度 h 被认为是一个重要参数,它控制着地球气候和大气化学成分的某些特征。还已知 h 在昼夜和季节时标上变化两个数量级。本简要说明着重指出了这种变异性对大气近地表气候和化学成分的影响。我们用准平衡 h 解释Budyko型能量平衡模型的热容量参数。分析表明,它是最浅的,分层稳定的,且具有最小的 h 的PBL,在气候模拟中应特别注意。讨论了PBL深度与温度(浓度)之间的相互依赖关系。分析特别指出,在稳定分层的PBL发作期间的气候特征应该对地球能量平衡和排放速率的扰动更加敏感。在此平台上,比较了来自ERA-40重新分析数据的 h ,CHAMP卫星产品和DATABASE64数据。 DATABASE64用于通过可用的气象剖面观测评估Troen-Mahrt方法来确定 h 。如之前所发现的,浅层PBL需要更好的参数化和更好的检索算法。研究表明,ERA-40和CHAMPdata在浅极性PBL中偏向更深的 h 。加上缺乏实地观测,可能会误导北极气候变化机制起源的归属。

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