ATMOSPHERIC GAS FLOW AROUND AND INSIDE HIGH HALLS SUPPORTED WITH THE SIMULATION OF THE FANS

Here we work with the system of equations describing the non-stational)) compressible turbulent multi-component flow in the gravitational field, and we focus on the numerical solution of these equations. The RANS equations are discretized with the use of the finite volume method. The exact solution of the modified Riemann problem (original results) is used at the boundary faces. The presented computational results are computed with the own-developed code (C, FORTRAN, multiprocessor, unstructured meshes in general).