We extract cases that are observed directly by satellite (TRMM 3B42 data) as well as well-analyzed in the precipitation produced by a global dynamical model (MERRA) which only assimilates wind and thermodynamic data. In order to narrow the scope of our investigation, we select case studies over the upper tropical latitudes of Asia. In each case (via selection off of a scatterplot of TRMM vs. MERRA rainfall), a standard, multivariate depiction of the atmosphere (centered on the event's spatial-temporal coordinates) is generated. Unidata’s Interactive Data Viewer (IDV) produces IDV "bundles" which fetch and render a set of thermodynamic and dynamical variables. We then individually examine these variables in IDV's interactive, more user-friendly interface. Case examples may also involve those when MERRA fails to analyze the TRMM-observed precipitation. However, future goals of simulation experiments will be best reserved for well-analyzed cases.
Preliminary findings show that favorable dynamics for large rainfall accumulations involve those that favor longevity and stationarity of storms (i.e. weak 500 hPa wind fields, terrain anchoring, high PWATs). While upper-level dynamical forcing is commonly found in mid-latitude systems, it is less frequent in cases of tropical convection. However, tropical cyclones are commonly included in extreme rainfall cases observed on these scales. In future work, we will classify related cases, average their fields into composites in order to discover systematic factors over cases whilst removing any case-specific anomalies. WRF simulations with modified initial conditions will then be utilized to test hypotheses that determine which are the more important factors in extreme rainfall accumulations.