TC simulations are conducted in a nonlinear shallow water model based upon a flexible dynamical core using either continuous or discontinuous Galerkin numerical methods (NUMA; Nonhydrostatic Unified Model of Atmosphere). The following experiments are examined, representing idealizations of TC processes in the real atmosphere: (i) a hurricane-like vortex advecting in a background flow, (ii) a dynamically unstable hurricane-like vortex, and (iii) and genesis of TC-like vortices from barotropic instability of a zonal jet. AMR versus non-AMR simulations are conducted for each case, and compared with each other for computational efficiency and accuracy. Moreover, large-level AMR experiments are conducted to demonstrate the utility of finely resolving small-scale features in the TC inner-core responsible for intensity variability.
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