Visualization with SDvision of ASH Stellar MHD Simulations

Numerical simulations are playing a leading role in the study of astrophysical objects. The ASH program is used to perform high-resolution three-dimensional simulations of the MHD processes occurring in the convection zone of the Sun and other stars. The size and complexity of the data produced in these simulations require to use special software tools at the post-treatment, visualization and analysis stages. The SDvision graphical interface is developed to provide an interactive and immersive visualization of such data. In this paper, we describe the different rendering capabilities provided by this program.