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A Multiresolution Ensemble Kalman Filter using Wavelet Decomposition

机译:一种基于小波分解的多分辨率集合卡尔曼滤波器

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摘要

We present a method of using classical wavelet based multiresolution analysisto separate scales in model and observations during data assimilation with theensemble Kalman filter. In many applications, the underlying physics of aphenomena involve the interaction of features at multiple scales. Blending ofobservational and model error across scales can result in large forecastinaccuracies since large errors at one scale are interpreted as inexact data atall scales. Our method uses a transformation of the observation operator inorder to separate the information from different scales of the observations.This naturally induces a transformation of the observation covariance and weput forward several algorithms to efficiently compute the transformedcovariance. Another advantage of our multiresolution ensemble Kalman filter isthat scales can be weighted independently to adjust each scale's effect on theforecast. To demonstrate feasibility we present applications to a onedimensional Kuramoto-Sivashinsky (K-S) model with scale dependent observationnoise and an application involving the forecasting of solar photospheric flux.The latter example demonstrates the multiresolution ensemble Kalman filter'sability to account for scale dependent model error. Modeling of photosphericmagnetic flux transport is accomplished by the Air Force Data AssimilativePhotospheric Transport (ADAPT) model.
机译:我们提出了一种基于经典小波的多分辨率分析方法,可以在通过集合卡尔曼滤波器进行数据同化的过程中分离模型和观测结果的尺度。在许多应用中,现象的潜在物理学涉及多个尺度上的要素相互作用。跨尺度的观测误差和模型误差的混合可能会导致较大的预测准确性,因为一个尺度的较大误差被解释为所有尺度的不精确数据。我们的方法使用观察算子的变换来将信息从不同尺度的观察中分离出来,这自然引起了观察协方差的变换,并提出了几种算法来有效地计算变换后的协方差。我们的多分辨率集成卡尔曼滤波器的另一个优点是,可以独立地对秤进行加权,以调整每个秤对预报的影响。为了证明可行性,我们将其应用于具有尺度依赖的观测噪声的一维Kuramoto-Sivashinsky(K-S)模型的应用以及涉及太阳光球通量预测的应用。光球磁通量传输的建模是通过空军数据同化光球传输(ADAPT)模型完成的。

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