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Ensemble filter based estimation of spatially distributed parameters in a mesoscale dust model: experiments with simulated and real data

机译:基于集合滤波器的中尺度尘埃模型中空间分布参数的估计:模拟和真实数据实验

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摘要

The ensemble adjustment Kalman filter (EAKF) is used to estimate theerodibility fraction parameter field in a coupled meteorology and dustaerosol model (Coupled Ocean/Atmosphere Mesoscale Prediction System (COAMPS))over the Sahara desert. Erodibility is often employed as the keyparameter to map dust source. It is used along with surface winds (or surfacewind stress) to calculate dust emissions. Using the Saharan desert as a testbed, a perfect model Observation System Simulation Experiments (OSSEs) with40 ensemble members, and observations of aerosol optical depth (AOD), theEAKF is shown to recover correct values of erodibility at about 80% of thepoints in the domain. It is found that dust advected from upstream gridpoints acts as noise and complicates erodibility estimation. It is also foundthat the rate of convergence is significantly impacted by the structure ofthe initial distribution of erodibility estimates; isotropic initialdistributions exhibit slow convergence, while initial distributions withgeographically localized structure converge more quickly. Experiments usingobservations of Deep Blue AOD retrievals from the MODIS satellite sensorresult in erodibility estimates that are considerably lower than the valuesused operationally. Verification shows that the use of the tuned erodibilityfield results in better predictions of AOD over the west Saharaand the Arabian Peninsula.
机译:集成调整卡尔曼滤波器(EAKF)用于在撒哈拉沙漠上的气象和尘埃气溶胶耦合模型(海洋/大气中尺度耦合预测系统(COAMPS))中估计可蚀性分数参数字段。可蚀性通常被用作绘制粉尘源图的关键参数。它与表面风(或表面风应力)一起用于计算粉尘排放量。使用撒哈拉沙漠作为测试平台,具有40个整体成员的完美模型观测系统模拟实验(OSSE)以及气溶胶光学深度(AOD)的观测,显示EAKF可在约80%的点上恢复正确的可蚀性值。发现从上游网格点平流的粉尘起噪声的作用,并且使可蚀性估计变得复杂。还发现收敛速度受可蚀性估计值初始分布的结构的显着影响。各向同性初始分布表现出缓慢的收敛性,而具有地理局部结构的初始分布则收敛更快。使用从MODIS卫星传感器获取的深蓝色AOD的观测进行的实验得出的可蚀性估算值明显低于可操作使用的值。验证表明,使用可调谐侵蚀性场可以更好地预测西撒哈拉和阿拉伯半岛的AOD。

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