Multiscale Data Assimilation Multiscale Dimensionality Reduction for Rainfall Fields Eulerian vs. Lagrangian Perspectives 1 Some Difficulties in Rainfall Assimilation model y precipitation truth truth model x time Rainfall Errors a Point: Perspective Chatdarong’s Approach from a at Lagrangian • Non-Gaussian, Non-smooth (Atomic Probability Mass) • • Position Errors (shift detection by MRA) Non-stationary • Scale (Intensity) Errors(2) Mis-timed events; (3) Missing/excessive (1) Mis-located rainfall cells/clusters; cells/events. • Timing Errors 2 Eulerian and Lagrangian Representations Eulerian Perspective Lagrangian Perspective Rasterization – Easy! c1 y Storm cell/cluster identification/ tracking (Quantization) – Difficult! c2 c4 c3 cluster1 x • Sequence of raster images (time series of points) • Clusters/cells, and their locations, shapes, sizes, intensities, life cycles, ... • High-dimensional, sparse • Low-dimensional, compact • Complicated errors • Less complicated errors • Implicit multiscale structures • Explicit multiscale structures • Most data available in this framework • No observation data in this format so far 3 Assimilation on an Implicit Multiscale Structure Implicit Multiscale Structure (from Chatdarong’s Thesis) 4 Assimilation on an Explicit Multiscale Structure Explicit Multiscale Structure Large Scale Features Storm Cells Radar Resolution 5 Available Storm Identification and Tracking Techniques NOAA: Storm Cell Identification and Tracking algorithm (SCIT) UCAR: Thunderstorm Identification Tracking Analysis and Nowcasting (TITAN) 6 RCR Model Developed at MIT 7 Storm Cell/Cluster Identification/Tracking 8 Storm Cell/Cluster Identification/Tracking 9 Storm Cell/Cluster Indentification/Tracking 10 Storm Cell/Cluster Indentification/Tracking 11 In Progress • Low dimensional representation and restoration. • Unsupervised algorithms. • Construction of likelihood function (error measure) for data assimilation. 12 End Thank You! 13 Backups from here on 14