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A multiresolution ensemble Kalman filter using the wavelet decomposition

机译:小波分解的多分辨率集成卡尔曼滤波器

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We present a method of using classical wavelet-based multiresolution analysis to separate scales in model and observations during data assimilation with the ensemble Kalman filter. In many applications, the underlying physics of a phenomena involve the interaction of features at multiple scales. Blending of observational and model error across scales can result in large forecast inaccuracies since large errors at one scale are interpreted as inexact data at all scales due to the misrepresentation of observational error. Our method uses a partitioning of the range of the observation operator into separate observation scales. This naturally induces a transformation of the observation covariance and we put forward several algorithms to efficiently compute the transformed covariance. Another advantage of our multiresolution ensemble Kalman filter is that scales can be weighted independently to adjust each scale's affect on the forecast. To demonstrate feasibility, we present applications to a one-dimensional Kuramoto-Sivashinsky (K-S) model with scale-dependent observation noise and an application involving the forecasting of solar photospheric flux. The solar flux application uses the Air Force Data Assimilative Photospheric Transport (ADAPT) model which has model and observation error exhibiting strong scale dependence. Results using our multiresolution ensemble Kalman filter show significant improvement in solar forecast error compared to traditional ensemble Kalman filtering.
机译:我们提出了一种使用经典的基于小波的多分辨率分析来分离模型和观测值的方法,该方法与集合卡尔曼滤波器进行数据同化。在许多应用中,现象的基础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误差,因为由于观测误差的错误表示,一个尺度上的大误差被解释为所有尺度上的不精确数据。我们的方法使用了将观察算子的范围划分为单独的观察标度。这自然会引起观测协方差的转换,因此我们提出了几种算法来有效地计算转换后的协方差。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,以调整每个秤对预测的影响。为了证明可行性,我们介绍了具有比例依赖的观察噪声的一维Kuramoto-Sivashinsky(K-S)模型的应用以及涉及太阳光球通量预测的应用。太阳通量应用使用空军数据同化光球传输(ADAPT)模型,该模型的模型和观测误差表现出很强的比例依赖性。与传统的集成卡尔曼滤波相比,使用我们的多分辨率集成卡尔曼滤波的结果显示出太阳预报误差的显着改善。

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