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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