[MGI28-P04] Development of a rotaging sphrical convection model for solving atmopspheric motions of the Jovian planets
Keywords:Jovian planets, anelastic system
For this purpose, we developed and parallelized an anelastic model of thermal convection in a rotating spherical shell considering basic radial density variation. The spectral transformation library used in this model was improved to introduce MPI parallelization not only in the latitude direction but also in the radial direction. As a result, we succeeded in increasing the number of parallel processes which had been limited by the number of latitudinal grid points, and more massive parallel numerical experiments became possible.