Code_Saturne solves the Navier-Stokes equations for 2D, 2D-axisymmetric and 3D flows, steady or unsteady, laminar or turbulent, incompressible or weakly dilatable, isothermal or not, with scalars transport if required. Several turbulence models are available, from Reynolds-Averaged models to Large-Eddy Simulation models. In addition, a number of specific physical models are also available as ”modules”: gas, coal and heavy-fuel oil combustion, semi-transparent radiative transfer, particle-tracking with Lagrangian modeling, Joule effect, electrics arcs, weakly compressible flows, atmospheric flows, rotor/stator interaction for hydraulic machines.
Keywords for this software
References in zbMATH (referenced in 3 articles )
Showing results 1 to 3 of 3.
- Ribés, Alejandro; Lorendeau, Benjamin; Jomier, Julien; Fournier, Yvan: In-situ visualization in computational fluid dynamics using open-source tools: Integration of Catalyst into \itCode_Saturne (2015)
- Archambeau, Frédéric; Hérard, Jean-Marc; Laviéville, Jér^ome: Comparative study of pressure-correction and Godunov-type schemes on unsteady compressible cases (2009)
- Eymard, R.; Herbin, R.; Latché, J.C.: Convergence analysis of a colocated finite volume scheme for the incompressible Navier-Stokes equations on general 2D or 3D meshes (2007)
Further publications can be found at: http://code-saturne.org/cms/community/references/articles