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A Composite View of Ozone Evolution in the 1995-1996 Northern Winter Polar Vortex Developed from Airborne Lidar and Satellite Observations

机译:从机载激光雷达和卫星观测结果得出的1995-1996年北部冬季极地涡旋中臭氧演化的综合观点

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摘要

The processes which contribute to the ozone evolution in the high latitude northern lower stratosphere are evaluated using a three dimensional model simulation and ozone observations. The model uses winds and temperatures from the Goddard Earth Observing System Data Assimilation System. The simulation results are compared with ozone observations from three platforms: the differential absorption lidar (DIAL) which was flown on the NASA DC-8 as part of the Vortex Ozone Transport Experiment; the Microwave Limb Sounder (MLS); the Polar Ozone and Aerosol Measurement (POAM II) solar occultation instrument. Time series for the different data sets are consistent with each other, and diverge from model time series during December and January. The model ozone in December and January is shown to be much less sensitive to the model photochemistry than to the model vertical transport, which depends on the model vertical motion as well as the model vertical gradient. We evaluate the dependence of model ozone evolution on the model ozone gradient by comparing simulations with different initial conditions for ozone. The modeled ozone throughout December and January most closely resembles observed ozone when the vertical profiles between 12 and 20 km within the polar vortex closely match December DIAL observations. We make a quantitative estimate of the uncertainty in the vertical advection using diabatic trajectory calculations. The net transport uncertainty is significant, and should be accounted for when comparing observations with model ozone. The observed and modeled ozone time series during December and January are consistent when these transport uncertainties are taken into account.
机译:使用三维模型模拟和臭氧观测资料评估了在高纬度北部低平流层中臭氧演化的过程。该模型使用来自戈达德地球观测系统数据同化系统的风和温度。将模拟结果与从三个平台上观察到的臭氧进行了比较:作为涡旋臭氧传输实验的一部分,差分吸收激光雷达(DIAL)在NASA DC-8上飞行;微波肢体测深仪(MLS);极地臭氧和气溶胶测量(POAM II)太阳掩星仪。不同数据集的时间序列彼此一致,并且与12月和1月的模型时间序列不同。结果表明,12月和1月的臭氧模型对模型光化学的敏感性比对模型垂直迁移的敏感性要低得多,后者取决于模型的垂直运动以及模型的垂直梯度。我们通过将模拟与臭氧的不同初始条件进行比较,评估了模型臭氧演变对模型臭氧梯度的依赖性。当极涡内12至20 km之间的垂直剖面与12月DIAL观测值非常吻合时,整个12月和1月的模拟臭氧最类似于观测到的臭氧。我们使用非绝热轨迹计算对垂直对流的不确定性进行定量估计。净输运不确定性很大,在将观测值与臭氧模型进行比较时应考虑在内。考虑到这些运输不确定性,在12月和1月观察到的臭氧时间序列和建模的臭氧时间序列是一致的。

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